Review article: Geothermal heat flow in Antarctica: current and future directions
- 1British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET, UK
- 2Alfred Wegener Institute – Helmholtz Centre for Polar and Marine Research, Am Alten Hafen, Bremerhaven, Germany
Correspondence: Alex Burton-Johnson (firstname.lastname@example.org)
Antarctic geothermal heat flow (GHF) affects the temperature of the ice sheet, determining its ability to slide and internally deform, as well as the behaviour of the continental crust. However, GHF remains poorly constrained, with few and sparse local, borehole-derived estimates and large discrepancies in the magnitude and distribution of existing continent-scale estimates from geophysical models. We review the methods to estimate GHF, discussing the strengths and limitations of each approach; compile borehole and probe-derived estimates from measured temperature profiles; and recommend the following future directions. (1) Obtain more borehole-derived estimates from the subglacial bedrock and englacial temperature profiles. (2) Estimate GHF from inverse glaciological modelling, constrained by evidence for basal melting and englacial temperatures (e.g. using microwave emissivity). (3) Revise geophysically derived GHF estimates using a combination of Curie depth, seismic, and thermal isostasy models. (4) Integrate in these geophysical approaches a more accurate model of the structure and distribution of heat production elements within the crust and considering heterogeneities in the underlying mantle. (5) Continue international interdisciplinary communication and data access.
The Antarctic ice sheet is the world's largest potential driver of sea level rise, and accurately modelling its dynamics relies, amongst others, on constraining conditions at the ice–bedrock interface. Measuring these basal conditions is inherently challenging and, of all the parameters affecting ice sheet dynamics, subglacial geothermal heat flow (GHF) is one of the least constrained (Larour et al., 2012; Llubes et al., 2006). Despite this uncertainty, GHF affects (1) ice temperature and, as a consequence, ice mechanical properties (rheology); (2) basal melting and sliding; and (3) the development of unconsolidated water-saturated sediments, all of which can promote ice flow (Greve and Hutter, 1995; Larour et al., 2012; Siegert, 2000; Winsborrow et al., 2010). Beyond ice dynamics, our knowledge of GHF allows us to model past and present basal melt rates in our exploration for old ice core climate records (Van Liefferinge et al., 2018), constrain models of glacial isostatic adjustment (GIA; van der Wal et al., 2013, 2015), and inform on the geological and tectonic development of Antarctica (McKenzie et al., 2005).
In recognition of the ambiguity and importance of Antarctic GHF, an increasing number of studies in geology, geophysics, and glaciology have sought to constrain this parameter, with a developing dedicated multinational interdisciplinary community (Burton-Johnson et al., 2019; Halpin and Reading, 2018). However, with an expanding research base and a requirement for multidisciplinary science, the necessity for a multidisciplinary review of current approaches and future directions was highlighted by the GHF sub-group of SERCE (Solid Earth Response and influence on Cryospheric Evolution) and the Scientific Committee on Antarctic Research (SCAR) (Burton-Johnson et al., 2019). This paper also provides the background material for a SCAR-commissioned white paper on future research directions (Burton-Johnson et al., 2020).
1.1 What is geothermal heat flow (GHF)?
GHF describes the transport of heat energy from the interior of the Earth to the surface (Gutenberg, 1959; Pollack et al., 1993). This heat originates from two primary sources: (1) the primordial heat remaining from the formation of the Earth, when the kinetic energy of celestial collisions was transformed into heat energy and (2) the radioactive decay of heat-producing elements (HPEs) and their isotopes, 98 % of which is derived from uranium, thorium, and potassium (Beardsmore and Cull, 2001; Lowrie, 2007). The HPEs are incompatible with the mineral structures of the mantle so are concentrated into the crust (Boden, 2016; McDonough and Sun, 1995). Other sources of possible contributions to GHF are (1) geoneutrino emission from the mantle (Huang et al., 2013; Korenaga, 2011) and (2) gravitational pressure (Elbeze, 2013; Morgan et al., 2016).
The estimated average heat flow of continental crust is 67.1 mW m−2, whilst for oceanic crust it is 78.8 mW m−2 (Lucazeau, 2019; although estimates vary according to sampling strategy and the number of observations). The difference between continental and oceanic heat flow reflects the smaller thickness of oceanic crust, with hot mantle rocks at comparatively shallow depths. Continental GHF varies significantly, primarily in response to variations in crustal heat production, age, composition, tectonic history, and thickness of crust and mantle (Mareschal and Jaupart, 2013). This results from the geological complexity of composite continental crust compared with oceanic crust. GHF is generally lower in stable crust away from convergent and divergent continental margins and rift basins and higher in these magmatically active provinces (Lucazeau, 2019; Pollack et al., 1993). On a broad regional scale, continental GHF correlates negatively with age, allowing first-order empirical estimation of Antarctic GHF based on its range of crustal ages (Fig. 1; Llubes et al., 2006; Sclater et al., 1980). However, Antarctic crustal heat production estimates show high variability across sampled age ranges (Gard et al., 2019), with lithology and tectonic setting being important controls on the heat production distribution (Carson et al., 2014; Halpin et al., 2019).
The rate of heat flow, Q, can be approximated by Fourier's law (Baron Fourier, 1822). In the simple model of a homogenous material with a constant thermal gradient, this equates to
where Q has the units milliwatts per square metre (i.e. power per unit area), T is the temperature (K), z is the vertical distance (m), and κ is the thermal conductivity of the material (mW m−1 K−1). When considering the basal conditions of the Antarctic ice sheet, we are interested in the heat flow at bedrock surface. We also need to consider internal heat production, A (µW m−3). For a simple case of constant thermal conductivity and heat production, surface heat flow can be described by
where the integral is measured from the surface to a depth, d (Eq. 1.13 in Beardsmore and Cull, 2001).
We would like to highlight here that most methods to estimate GHF derive it from the temperature gradient, as in Eqs. (1) and (2). However, these equations are a simplification, as temperature variation over time, surface topography, internal heat production, and variation in the properties of the material all affect the observed temperature gradient.
1.2 A note on terminology: heat “flow” vs. heat “flux”
In the scientific literature, heat flow and heat flux are used interchangeably. The consensus from the SCAR-SERCE white paper authorship (Burton-Johnson et al., 2020) is that flow is the correct terminology. Heat flow is not limited to the movement of material, but the mechanism of heat transfer (dominantly by conduction when near the Earth's surface). Although the two terms are used interchangeably, heat flow has been established for decades to describe the rate of heat transferred across the surface of Earth per unit area, is the term used by the International Heat Flow Commission, and is thus the term used here. We recommend adopting this term in preference in the future, although the most important consideration is to state the correct units (mW m−2).
GHF can strongly influence the basal temperature of the ice sheet. As a consequence, it is a key contributor to basal meltwater production, ice rheology, basal friction, basal sliding velocity, and erosion (Fahnestock et al., 2001; Goelzer et al., 2017; Hughes, 2009).
The heat budget at the base of an ice sheet can be described (Vieli et al., 2018) as
where Qg is the GHF, Qs is the heat generated by sliding, Qw is the heat generated by subglacial water flow, Qp is the heat required to maintain the flowing water at pressure melting point, Qf is the heat released by freezing or used by melting and Qc is the heat conducted away in the ice towards the ice surface. Of the positive contributions to basal heat, that generated by sliding (Qs) can be orders of magnitude greater than that from GHF (Qg), but in slow-flowing areas Qs is negligible and GHF plays a key role in the heat budget (Larour et al., 2012; Pittard et al., 2016a).
To illustrate this point, Llubes et al. (2006) modelled a 20 mW m−2 increase in GHF across the Antarctic continent (from uniform values of 40 to 60 mW m−2). This resulted in a 6 ∘C increase in the mean basal temperature, from −13 to −7 ∘C, and expanded the proportion of the basal ice area above the pressure melting point (PMP) from 16 % to more than 50 %. This variation directly affects the basal melt rates, with a uniform 40 mW m−2 generating 6.7 km3 yr−1 of basal melting across Antarctica, whilst 60 mW m−2 would generate 18 km3 yr−1. However, unlike the GHF values used, the resultant basal temperature variation is non-uniform: although the two heat flow models produce only a few degrees Celsius difference in basal temperature near the coast, they generate up to 15 ∘C difference in central East Antarctica. This is because horizontal advection and frictional basal heating are negligible beneath the thick, slow-moving ice of East Antarctica, and surface temperatures have a reduced effect on basal conditions (Llubes et al., 2006; Pollard et al., 2005). In these regions of thick ice, the increased pressure brings the basal ice temperature closer to its PMP (Pollard et al., 2005), and the thicker ice has a greater insulating effect. Although the effect of pressure of basal temperature is much smaller than surface temperature variation, in areas of thick ice where the basal temperature is close to the PMP, even small variation in GHF can determine whether basal melting occurs. This has a resultant effect on the basal friction and sliding of the ice sheet (Pollard et al., 2005). In addition, the increased ice temperature makes it more susceptible to internal deformation, which also enhances its ability to flow (Llubes et al., 2006).
Even beneath the comparatively thinner ice of West Antarctica, the sensitivity of basal temperature to heat flow is enhanced (Llubes et al., 2006). There is evidence that this region, dominated tectonically by the West Antarctic Rift System (Jordan et al., 2020), exhibits very high values of basal heat flow and resultant basal melting (Schroeder et al., 2014). Above 85 mW m−2, the basal temperature of much of the West Antarctic Ice Sheet will pass its pressure melting point (in agreement with radar evidence for extensive basal melting; Llubes et al., 2006; Rémy and Legresy, 2004; Schroeder et al., 2014). Consequently, enhanced basal heat flow in West Antarctica can have a large effect on its basal melt rates, although the thinner ice sheet in West Antarctica compared to East Antarctica makes it more sensitive to surface parameters (advection and conduction of the surface temperature, itself influenced by the accumulation rate; Llubes et al., 2006).
In addition to enhancing basal melting and reducing basal friction, increased GHF enhances ice flow by increasing the englacial temperature and thus reducing the ice stiffness (Larour et al., 2012). Because the heat produced by basal friction and viscous deformation can be orders of magnitude greater than from GHF in fast-flowing ice streams, this effect is only significant in upstream, slow-flowing areas (Larour et al., 2012). In these regions of thick, slow-flowing ice, even local high heat flow anomalies of insufficient heat for basal melting can result in the development of accelerated, channelized flow for hundreds of kilometres upstream and downstream of the GHF anomaly through the effect of GHF on the ice rheology (Pittard et al., 2016a). Regions along ice divides and adjacent to ice streams are particularly sensitive to enhanced GHF (Pittard et al., 2016b).
Whilst the points above highlight the necessity of estimating Antarctic GHF, it is very important that the accuracy of these estimates can be verified. The impact of inaccurate GHF constraints on models of ice sheet dynamics has been shown by comparing GHF estimates for Greenland. Ice sheet modelling controlled by spatially variable GHF forcing reproduces the observed state to only a limited degree and fails to reproduce either the topography or the low basal temperatures measured in southern Greenland (Rogozhina et al., 2012). Instead, an unrealistic spatially uniform GHF forcing produces a considerably better fit. If the much larger Antarctic ice sheet is to be accurately modelled, the accuracy of the GHF estimates used must be well constrained by multiple independent methodologies, sensitivity tests, and comparison of different models.
Recently, there has been increasing interest in the exploration of suitable locations for coring Antarctica's oldest continuous ice record (Fischer et al., 2013). This problem requires accurate knowledge of GHF, as basal melt rates limit the maximum possible age of recoverable ice (Van Liefferinge et al., 2018). Additionally, due to environmental concerns around possible drilling fluid contamination, frozen bed conditions are a prerequisite for deep-coring operations for recovery of the oldest ice records.
2.2 Glacial isostatic adjustment (GIA)
The temperature of the lithosphere and upper mantle are important parameters for modelling the isostatic response to changes in the volume of the overlying ice sheet (i.e. glacial isostatic adjustment, GIA). This is because the (visco)elastic properties of the lithosphere and mantle directly relate to its thermal properties (Chen et al., 2018; Kuchar and Milne, 2015). GIA is a critical component of the long-term evolution of ice sheets and could potentially stabilize retreating ice streams in submarine settings (Barletta et al., 2018; Kingslake et al., 2018). Of particular importance here is that the temperature-dependant viscosity that controls GIA can be modelled using surface heat flow estimates (van der Wal et al., 2013, 2015).
2.3 Geology and tectonics
2.3.1 Mantle dynamics
Heat flow variation and its isostatic effects (i.e. the buoyancy control on crustal elevation, resulting from the different densities of the dense mantle and less dense overlying crust) provide evidence for mantle dynamics beneath a continent. For example, high heat flow anomalies have been proposed as evidence for sub-lithospheric heating by present and past mantle plumes (regional hotspots of warm mantle upwelling beneath the lithosphere; e.g. Courtney and White, 1986; Martos et al., 2018), and the absence of enhanced heat flow where mantle ascent is proposed has been used to argue against such processes (e.g. Stein and Stein, 2003). Also, because of the relationship between surface heat flow and isostatic elevation, heat flow studies can reveal thermal or compositional variation in the sub-continental mantle, as a reduction in its density can increase the isostatic elevation of the surface topography (Hasterok and Gard, 2016).
2.3.2 Development of the lithosphere
The thermal properties of the lithosphere control its response to tectonic deformation (e.g. Sandiford and Hand, 1998), such as the development of crustal shear zones and earthquakes. The lithosphere's thermal properties also affect the relative density of lithosphere and underlying mantle and (as a result of this buoyancy effect) the isostatic surface elevation. This in turn influences the heights of Antarctica's mountain ranges and the depths of its sedimentary basins (McKenzie et al., 2005). For these reasons, understanding the continent's GHF will inform on the development of many of Antarctica's largest tectonic features. For example, the lithospheric extension of the West Antarctic Rift System, the prominent elevation of the Transantarctic Mountains, the deep topographic depression of the Wilkes subglacial basin, and the extensive Palmer Land Shear Zone of the Antarctic Peninsula.
Having highlighted the importance of constraining Antarctica's GHF, the following sections discuss current approaches to its estimation. The methods discussed are summarized in Table 1.
Local heat flow estimates can be derived by measuring the temperature at various depths below the surface (in either the bedrock, overlying sediments, or sheet) and deriving a temperature gradient. In Antarctica, GHF has been derived through temperature measurements from boreholes into the bedrock or into the ice sheet and also from probes into unconsolidated sediments. It is important to recognize that these are “estimates” not “measurements” of GHF, particularly when using them to verify the accuracy of geophysical or inverse GHF estimates. This is because the measured thermal gradient can be affected by processes other than GHF, including surface temperature variation and hydrothermal circulation. When evaluating a specific local estimate, its derivation, local geology, and other regional GHF estimates must be considered. Thermal gradients and surface heat flow may vary significantly over 10 km lateral spatial resolutions (Carson et al., 2014) with variations in geology (affecting heat production and conductivity; Carson et al., 2014; Hasterok and Chapman, 2011), hydrothermal circulation (affecting local heat convection and redistribution; Fisher and Harris, 2010), and topography (affecting heat diffusion pathways to the surface; Bullard, 1938; Lees, 1910).
3.1 Boreholes into bedrock
The thermal gradient can be determined by measuring the temperature variation at different depths in the crust. Away from Antarctica, these measurements are from boreholes (commonly those drilled for mineral or hydrocarbon exploration), mineshafts, caves, or other cavities. The temperature gradient of the crust's uppermost 10–50 m is dominantly affected by downward conduction of the surface temperature rather than GHF. To address this, temperature measurements are made over the largest depth range possible (typically 100–1000 m).
Borehole temperature measurements are made using wire-line temperature probes, with a thermistor at the leading tip and measurements made progressively downwards to minimize disturbance of the borehole fluids prior to temperature measurement. The temperature is measured from the bore fluid, not the surrounding rock, so an important consideration is the need for thermal equilibration of the wall rock and the borehole fluids following drilling and prior to measurement. In addition, the heat produced during drilling needs to be dissipated from the borehole. As a guide, 10–20 times the drilling time is required before a borehole is equilibrated to within instrument accuracy (Bullard, 1947; Jaeger, 1956), although observations show that after 3 times the drilling time, borehole fluids are within 0.05 ∘C of equilibrium values (Lachenbruch and Brewer, 1959). As an example of the time required for bedrock drilling, drilling of the multiple Cape Roberts Project boreholes averaged 16–31 m d−1 (Talalay and Pyne, 2017). For the low water flows used in small-core (<4 cm diameter) diamond drilling (compared with the high water flows of wider core diameter rotary drilling), heat exchange is negligible except for the upper- and lowermost ∼20 % of the borehole, and full temperature profile measurements can be taken about 2 d after drilling cessation (Jaeger, 1961, 1965).
Depth below the bedrock surface must be considered when taking borehole temperature measurements. Where terrestrial bedrock is exposed, atmospheric temperature and seasonal variation perturbs the thermal gradient in the upper >100 m of the crust. In Antarctica, temperatures from Hole 3 of the Dry Valley Drilling Project provided estimates of “equilibrium” gradient only when deeper than 90 m (Decker, 1974; Decker et al., 1975; Pruss et al., 1974). It may be possible to compensate for seasonal variation in shallower boreholes using long-term observations of the temperature gradient (>1 year), although the previous attempt (from a 7.6 m borehole at McMurdo Station; Risk and Hochstein, 1974) derived an anomalously high GHF estimate (164 mW m−2, compared to 66 mW m−2 from a 260 m deep borehole; Decker and Bucher, 1982).
Subglacial bedrock is not exposed to atmospheric temperature variation, so the geothermal gradient can be measured from shallower depths. However, it is affected by heat derived from the overlying ice sheet: internal and basal frictional shear heating from the ice sheet, heat advection, basal water, and seasonal temperature variation (e.g. Ritz, 1987). In the absence of a deep, borehole-derived, subglacial bedrock temperature profile, the depth required to accurately measure the unperturbed geothermal temperature gradient is currently unknown. Thermal diffusion modelling over timescales of low-frequency climate variation may constrain this.
3.2 Ice boreholes
Subglacial GHF can be estimated from the temperature gradient from boreholes into the ice sheet (e.g. Engelhardt, 2004; Fudge et al., 2019; Nicholls and Paren, 1993). This requires that there is no additional heating from basal shear or horizontal advection and that the ice sheet has been unequivocally frozen to the bed for long enough that the bedrock and overlying ice sheet have thermally equilibrated. To meet this requirement, the temperature profile is best measured from cores into the summits of ice domes where the ice sheet is stationary (Engelhardt, 2004). As applies to bedrock boreholes, a delay between drilling and temperature measurement is required for the thermal disturbance from the drilling to dissipate. For hot-water drilling, this can take 2 years (Barrett et al., 2009; Engelhardt, 2004). The temperature profile is typically measured using thermistors, recording the temperature through changes in resistivity to electrical currents. Either a string of thermistors is deployed into the borehole prior to freezing, and the temperature is recorded over time, or the hole can be kept open with drill fluid and downhole temperature can be measured with a moving thermistor. More recently, temperature has also been recorded using distributed temperature systems (DTSs; Suárez et al., 2011; Ukil et al., 2011). The temperature is derived from the travel time of a laser beam within an optical fibre. All of these methods require thermal equilibration.
Once the englacial temperature profile is obtained, GHF estimation can be achieved through three methods. Firstly, if the borehole reaches the ice–bedrock interface, and the bedrock and overlying ice are in thermal equilibrium, then the GHF can be estimated in the same way as for bedrock boreholes (e.g. Engelhardt, 2004), that is, using the temperature gradient in the ice near the ice–bedrock interface but using the thermal conductivity of ice rather than rock (Eq. 1). Secondly, rather than measuring a temperature profile above the bed, the basal temperature at the ice–bedrock interface can be measured, and temperature can be modelled through time to constrain the required GHF (e.g. Fudge et al., 2019). Thirdly, if the borehole does not reach bedrock, similarly to the previous method a thermal model is required to constrain GHF (e.g. Zagorodnov et al., 2012) In the methods where modelling is required, the variables are modified within constraints determined for the location until the modelled temperature profile best fits the measurements (Fig. 3) and the modelled temperature gradient within the bedrock used for GHF calculation.
In regions where the ice sheet is frozen to the bed and thermally equilibrated, GHF can be estimated from boreholes that do not reach the bedrock, providing that the temperature profile is obtained below the penetration depth (or skin depth, δ) of surface temperature variation into the ice sheet. This depth is defined by the circular frequency of the variation (ω) and the thermal diffusivity of the material (k) according to Eq. (4) (Fig. 4; Carslaw and Jaeger, 1959; Wangen, 2010).
Here circular frequency (ω) is defined by Eq. (5), where tp is the time for one period (or cycle) of the temperature variation (Wangen, 2010).
The deepest significant perturbations of the englacial temperature profile are from glacial–interglacial cycles, and GHF is best estimated from the englacial temperature profile below the depth at which this effect becomes negligible. In Greenland, this is the bottom 20 % of the ice sheet, but in areas of low-accumulation in Antarctica this can extend to much shallower depths. With sufficiently accurate temperature measurements, the full temperature profile of the ice sheet and the subglacial GHF may be estimated from boreholes penetrating only the upper 600 m or 20 % of the total ice sheet thickness (Hindmarsh and Ritz, 2012; Mulvaney et al., 2019; Rix et al., 2019). However, shallow boreholes to estimate GHF use simplified thermal models and assumptions on ice sheet evolution, and so require further validation.
However, poorly constrained thermal effects within the ice sheet propagate uncertainties in GHF estimates from ice sheet boreholes (Cuffey and Paterson, 2010, chap. 9). This is a particular problem if there is any ambiguity as to whether the ice sheet is frozen to the bed. The englacial temperature profile depends on heat sources at the surface, base, and within the ice (i.e. internal deformation-derived frictional heating). Heat sources that act at the base of the ice, such as frictional heating by basal motion, are impossible to differentiate from GHF.
3.3 Marine and onshore unconsolidated sediments
Shallow ( m) temperature gradients in unconsolidated sediments can be recorded using gravity-driven probes rather than drilled boreholes. They carry multiple thermistors along the length of the probe that provide a temperature profile. These measurements can be taken from unconsolidated sediments offshore (e.g. Dziadek et al., 2019, 2017), in subglacial lakes (Fisher et al., 2015), or below ice shelves (Begeman et al., 2017).
As applies to borehole measurements, temperature gradients in unconsolidated sediments must be taken at sufficient depth to represent the crustal temperature gradient and not be perturbed by temperature variation in the overlying water or ice (i.e. they must be representative of steady-state conditions). The penetration depth of temperature variation is dependent on its frequency (Eq. 4 and Fig. 4; Carslaw and Jaeger, 1959). Consequently, diurnal or annual cycles only affect the upper few centimetres to couple of metres of the surface temperature profile, whilst variations over the last 200–300 years will affect the upper 200 m, and post-glacial warming can be observed down to 2500 m. These effects are dampened by an overlying water column or ice sheet, but temperature variation over 10 kyr can still affect basal ice sheet temperatures (Engelhardt, 2004). Although large (>10 ∘C) seasonal temperature variations are dampened by ∼90 % at water depths of 3–5 m (Müller et al., 2016), long-term variations (e.g. climate-controlled variations in Circumpolar Deep Water over the last ∼12 kyr; Hillenbrand et al., 2017) are likely recorded in the upper 3 m at 400 m water depth, 2 m at 700 m depth, and even the upper ∼1 m at 1000 m depth (Dziadek et al., 2019).
Similarly to borehole temperature measurements, a time delay must be considered between penetration of the sediments and temperature measurement. A 10 min delay between sediment penetration and measurement is sufficient to allow decay of frictional heating, as the temperature decay takes ∼100 s (Dziadek et al., 2019; Pfender and Villinger, 2002).
Unconsolidated temperature measurements can also be taken from marine boreholes (e.g. IODP boreholes). For bedrock boreholes, a delay is required between drilling and measurement for thermal equilibration of the wall rock and the borehole fluids, which would be problematic for marine boreholes where a drill ship cannot remain on site. Instead, for boreholes into unconsolidated sediments, a probe is deployed into the borehole bottom sediments shortly after drilling. Although technology has improved (Davis et al., 1997; Heesemann et al., 2006), measurements can be affected by frictional heating during and after probe deployment, or by movement of water and sediments within the hole. Only measurements that exhibit the expected temperature decay rate after penetration are thus reliable (Hyndman et al., 1987).
In addition to the few and sparse penetrative GHF estimates in Antarctica, continental (Fig. 5) and regional (Fig. 6) estimates have been derived from both solid Earth (geophysical/geological) and glaciological data and models.
4.1 Magnetically derived estimates
As for the penetrative methods of GHF estimation described above (Sect. 3), geophysical methods also derive GHF from a temperature gradient. In this case, magnetic survey data are used to determine the depth at which the maximum temperature of ferromagnetic magnetization is exceeded (the Curie temperature; Haggerty, 1978). This Curie temperature is different for different minerals but is assumed in these studies to be the Curie temperature of magnetite (580 ∘C) as this mineral is most commonly the dominant contributor to crustal magnetization (Bansal et al., 2011; Fox Maule et al., 2005; Langel and Hinze, 1998).
Above the Curie temperature, rocks lose their ability to maintain ferromagnetic magnetization (e.g. Haggerty, 1978). The depth of this isotherm in the crust (the Curie point depth, CPD; Figs. 7 and 2) is thus assumed to be the depth to the bottom of the magnetic source (DBMS) determined from magnetic survey data. The DBMS maps a transition zone, rather than an exact depth (Haggerty, 1978) and can provide information on crustal temperatures at depths not accessible by other means (Andrés et al., 2018; Okubo et al., 1985). Regions found to have a shallower DBMS (and thus an assumed shallower CPD) are expected to have higher average temperature gradients, and, therefore, higher GHF (e.g. Aboud et al., 2011; Andrés et al., 2018; Arnaiz-Rodríguez and Orihuela, 2013; Bansal et al., 2013, 2011; Bhattacharyya and Leu, 1975; Guimarães et al., 2013; Li et al., 2017; Obande et al., 2014; Okubo et al., 1985; Ross et al., 2006; Salem et al., 2014; Tanaka et al., 1999; Trifonova et al., 2009).
The first Antarctic-wide magnetically derived GHF map (Fox Maule et al., 2005; updated by Purucker, 2012, Fig. 5a) used the “equivalent source magnetic dipole method” (Mayhew, 1979) to map magnetic anomalies from multiple satellites at different altitudes as evenly distributed magnetic dipoles on the Earth's surface (Dyment and Arkani-Hamed, 1998). Due to filtering of the data during processing, this magnetic anomaly distribution is only susceptible to shallow, short-wavelength magnetic variation. To calculate the CPD, a long-wavelength CPD model was modified until it reproduced the determined short-wavelength anomalies. The temperature gradient represented by this CPD was combined with assumed homogenous crustal properties (heat production and conductivity) to model the surface heat flow. Due to the high altitude of the satellite data, the horizontal resolution of this approach was limited to at least a few hundred kilometres.
Spectral methods are the alternative and more commonly applied approach to estimating the DBMS, analysing the spectrum of wavelengths in magnetic profiles or gridded data (e.g. Blakely, 1996; Okubo et al., 1985; Spector and Grant, 1970). These methods depend on the implicit assumption that long-wavelength features result from deep sources. The depth of this source is calculated from a “power spectrum” (Fig. 8) of wavenumber (the inverse of the wavelength) against the logarithm of each wavenumber's “power” (the square of each wavelength's magnitude after conversion by a fast-Fourier transformation to describe the spectrum of wavelengths in the signal). From this power spectrum (Fig. 8) the top (Zt) and centre (Z0) of the deepest magnetic layer are inferred from the slope of the intermediate and long-wavelength zone of the spectra derived from magnetic anomaly data. The DBMS (ZDBMS) stems from the simple geometric relationship between these depths:
To map the DBMS across a study area, the spectra of magnetic anomalies are computed within overlapping rectangular windows regularly spaced over the aeromagnetic map. Particularly for gridded data, the dimensions of the region chosen to analyse the long-wavelength frequencies must be sufficiently large to capture the DBMS. Ravat et al. (2007) elaborate that the dimension of the region analysed may need to be (in some cases) up to 10 times the DBMS but that dimensions exceeding 200 to 300 km may average different large-scale crustal structures. This suggests that satellite data, which typically detect magnetic anomalies in that wavelength, may not be suitable for this spectral method of CPD estimation. Choosing the window size therefore forces a trade-off between accurately determining the DBMS within each sub-region and resolving small changes in DBMS between sub-regions (Ross et al., 2006).
Spectral methods have been applied in Antarctica (Dziadek et al., 2017; Martos et al., 2017; Purucker and Whaler, 2007; Figs. 5b and 6) to combined satellite and airborne magnetic anomaly data (e.g. ADMAP; Golynsky et al., 2006; Maus, 2010). The results show a general agreement at a continental scale but vary significantly on a regional scale (Fig. 5). This is related to the resolution of the magnetic anomaly data, particularly in regions where only satellite magnetic data are available. Furthermore, regional-scale magnetic anomaly databases are usually a mosaic of individual aeromagnetic surveys. Ross et al. (2006) emphasize that subtle discontinuities along survey boundaries are caused by differences in survey specifications, such as flight line spacing, flight altitude, regional field removal, or the quality of data acquisition. These, for instance, may contaminate the long-wavelength signal caused by deep magnetic sources (Grauch, 1993). Long-wavelength features can also result from shallow but spatially extensive sources, such as volcanic provinces, and can lead to an underestimation of the DBMS.
CPD estimates assume a homogenous magnetic mineralogy of magnetite and thus a Curie temperature of 580 ∘C (Bansal et al., 2011; Fox Maule et al., 2005; Langel and Hinze, 1998). This assumption neglects the compositional variability in plutonic rocks that lead to Curie temperature ranges between 300 and 680 ∘C and in cases of magnetic assemblages of Fe–Ni–Co–Cu metal alloys up to 620 to 1084 ∘C (Haggerty, 1978). Without further constraints and validations, these assumptions remain the best approach, especially in sparsely sampled regions like Antarctica, but they introduce uncertainties of several kilometres in Curie depths and consequent uncertainties in GHF estimates (Bansal et al., 2011; Ravat et al., 2007). Similarly, in areas of thin crust, non-magnetic mantle rocks can be shallower than the Curie depth. In these regions, the calculated CPD will appear shallower due to a lack of magnetic minerals in the mantle rocks (Fig. 9; Frost and Shive, 1986; Wasilewski and Mayhew, 1992). This can be investigated through comparison of the Antarctic Curie depth estimates with the seismically or gravitationally derived depth of the crust–mantle boundary (the Moho depth; Fig. 10 and Fig. 2). For example, thermal modelling of seismic, gravity, and magnetic data showed the DBMS of the Norwegian margin reflected the basement geometry, not the CPD, and that surface heat flow estimates using magnetic CPD models were thus unreasonably high (Ebbing et al., 2009).
However, whilst in general the Earth's mantle does not contribute to the magnetic signal (due to its weak magnetization and high temperature conditions), in some cases the Curie depth may indeed lie within the mantle. This occurs where metallic magnetic phases in the mantle beneath old, tectonically stable crust (“cratons”; Ferré et al., 2013) or subduction regions (e.g. Blakely et al., 2005) contribute to mantle magnetization. In these settings the crust–mantle boundary should not be considered an absolute magnetic boundary (Ferré et al., 2013). This implies that if in a given region the Moho depths are shallower than the deepest magnetic layer, a magnetic mantle at temperatures below the Curie temperature may be considered. However, even in these cases the upper mantle susceptibility will be more than 1–2 orders of magnitude smaller than the overlying crust. This is not considered in current spectral methods assuming constant susceptibility. Consequently, Curie depth methods yield non-unique solutions, and further available constraints and observations need to be considered, when interpreting the Curie temperature distribution (e.g. geological evidence, borehole measurements, and Moho depth estimates).
4.2 Seismically derived estimates
Temperature is the dominant control on seismic velocity in the mantle (e.g. Carlson et al., 2005), and hence the mantle heat flow at the base of the Antarctic crust can be determined from seismic data. By determining the change in seismic velocities marking the density discontinuity at the lithosphere–asthenosphere boundary (Fig. 2), the depth of the 1330 ∘C isotherm can be estimated. This is the “mantle adiabat” marking the top of the seismic low-velocity zone and the change from a solid to ductile mantle (Fig. 2). The continental-scale GHF can then be estimated by assuming the heat production and conductivity of the lithosphere above this boundary and integrating this with the seismically derived mantle heat flow (An et al., 2015b; Fig. 5d). However, the seismically derived, continent-scale Antarctic GHF model of An et al. (2015a) (Fig. 5d) is limited to a lateral spatial resolution of >120 km, assumes a laterally uniform crustal structure, and is insensitive to the lithospheric geotherm (instead it inversely correlates with crustal thickness).
Composition also affects seismic velocities. For example, a 2 % increase in velocity can be explained by either a 120 ∘C decrease in temperature, a 7.5 % depletion in iron, or a 15 % depletion in aluminium (Godey et al., 2004). Slow mantle velocities at subduction zones can also be caused by water or hydrous fluids serpentinizing the mantle wedge (Fig. 2; Kawakatsu and Watada, 2007). However, velocity in the Antarctic seismic model (An et al., 2015b) does not account for variability of mantle compositions, mineralogy, grain size, or water content of the mantle or crust. An uncertainty in the lithospheric thickness of 15–30 km was assumed by (An et al., 2015b) based on the 150 ∘C temperature uncertainty, but an ∼50 km uncertainty for ∼200 km thick lithosphere may me more accurate (Artemieva, 2011; Godey et al., 2004). In addition, seismological models suffer from limited and inconsistent spatial coverage, which can lead to discrepancies in upper-mantle velocities and differences in Moho depths (Fig. 2) up to 10 km, even for the same receiving station (supporting information of An et al., 2015b; Pappa et al., 2019b).
Some constraints on the mantle and lithosphere composition can be determined from xenoliths (rock fragments of the deep crust or mantle entrained in magma rising from depth) or exposed deep crustal sections, where variation in temperature and composition with depth can be determined from the metamorphic minerals present. Constraints can also be derived empirically by comparing the seismic velocity with similar regions. Shapiro and Ritzwoller (2004) (Fig. 5c) extrapolated global heat flow measurements to Antarctica based on the assumption that structurally similar regions have similar magnitudes of GHF. This was achieved by calculating a spatially variable “similarity functional” determined from the differences between the seismic velocity and seismic Moho depth between a location of interest and a comparable location elsewhere. A histogram of heat flow measurements could then be assigned to the location of interest in Antarctica based on the similarity-weighted sum of measurements from structurally similar regions and the mean values of these distributions mapped as continental heat flow. Spatial resolution was limited to the lateral resolution of the global shear velocity model across Antarctica (600–1000 km; Shapiro and Ritzwoller, 2002). Although the studies of Shapiro and Ritzwoller (2004) and An et al. (2015a) both used seismic data and are thus frequently compared, it is important to highlight that they use very different approaches in deriving heat flow (the former employing a probabilistic approach and the latter using forward modelling).
The empirical seismically derived model for Antarctica has recently been revised (Fig. 5d; Shen et al., 2020). Rather than the low-resolution global database used by Shapiro and Ritzwoller (2004), an Antarctic seismic model was derived and compared with the high-resolution seismic model and GHF measurements of the USA, again calculating spatially variable similarity functionals to compare the data. Recognizing the non-unique solutions provided by this method, Shen et al. (2020) also map the associated uncertainties of their model.
4.3 Gravity model-derived estimates
Satellite gravity data have been used as an alternative to seismic modelling to determine crustal thickness. Pappa et al. (2019b) used satellite gravity data, a model of global gravity variation (the “geoid”), surface and bedrock topography, and assumed rock and ice densities to calculate the topographically corrected variation in gravity in Antarctica (the “Bouguer anomaly”), from which the depth of the crust–mantle boundary could be calculated. This approach to calculate crustal thickness is sensitive to long-wavelength (>150 km) features representing deep structures, rather than short-wavelength, near-surface density changes. However, gravity-modelling solutions are non-unique and require additional constraints on the density contrast between the crust and mantle at a reference depth and/or seismic depth constraints on crustal thickness.
Using the gravity-derived crustal thickness estimates, cross-sectional models of the mantle and lithospheric structure were calculated, with adjustments made to crustal density and crustal thickness until the models reflected the observed variation in gravity and elevation (Pappa et al., 2019b). By assigning assumed values of heat productivity and thermal conductivity values to the modelled cross sections, surface heat flow was calculated along the line of the modelled cross section (Fig. 6).
4.4 Conjugate margin-derived estimates
An alternative approach to constrain the probable GHF of East Antarctica is to compare it with its Gondwanan conjugate margins, reconstructed prior to the breakup of the supercontinent (Fig. 11). Plate tectonic reconstructions indicate that the subglacial geology of East Antarctica is comparable to the margins of Australia, Africa, and India (Aitken et al., 2016; Daczko et al., 2018; Ferraccioli et al., 2011; Flowerdew et al., 2013; Mulder et al., 2019). By kriging the heat flow measurements of the continents in their pre-Gondwana breakup arrangement, Pollett et al. (2019) interpolated a heat flow surface through Antarctica and its conjugate margins (Fig. 11). This method highlighted similarities and differences between the most recent seismic and magnetically derived geophysical models of Antarctic heat flow (An et al., 2015b; Martos et al., 2017) with the better constrained heat flow of the conjugate margins. In particular, this approach showed reasonable agreement along the margin with Africa, but an absence in either the magnetic or seismic models of high-heat-flow provinces in East Antarctica comparable with south Australia, an absence of the low heat flow of SW Australia in the magnetically derived model of East Antarctica (Martos et al., 2017), and an absence of the high heat flow of northern India in the seismically derived model of East Antarctica (An et al., 2015b). However, when extrapolating heat flow away from the conjugate margins into the interior of Antarctica, this approach is susceptible to the method of interpolation used and the quality and scarcity of the borehole-derived GHF estimates in the interior of Antarctica (Sect. 3).
4.5 Isostatic elevation
In addition to crustal thickness and density, the thermal state of the lithosphere also contributes to its isostasy and observed surface elevation. The effect of thermal isostasy on the bathymetry of oceanic crust is well recognized: as oceanic crust migrates from the spreading ridge it cools, thickens, contracts, and subsides (Stein and Stein, 1992). However, the effect of thermal isostasy on continents is masked by compositional contributions to isostatic elevation (i.e. lateral variations in crustal thickness and density, Fig. 12a; Hasterok and Chapman, 2007a, b).
Hasterok and Chapman (2007a, b) developed a methodology for investigating thermal isostasy in the continental lithosphere by normalizing the observed elevation using an isostatic correction. The calculated compositionally corrected elevation generally increases with increasing surface heat flow (Fig. 12b). This approach was used to derive the thermal contribution to isostatic elevation of Australia and North America and estimate the continental sub-lithospheric and radiogenic heat flow (Hasterok and Chapman, 2007b; Hasterok and Gard, 2016). Whilst in general the compositionally corrected elevation and surface heat flow values followed the modelled curve for thermal isostatic equilibrium (Fig. 12b), anomalous regions lie away from this curve. These anomalies result from (1) additional sources of buoyancy and/or dynamic support (e.g. anomalously buoyant mantle lithosphere); (2) anomalous surface heat flow, not representative of the deeper thermal regime (e.g. high concentration of heat-producing elements in the shallow crust); (3) deviations from the thermal properties of the reference crustal model (e.g. heat production); or (4) combinations of these properties (Hasterok and Gard, 2016).
Although developed for regions of known heat flow, application of this approach to Antarctica (Hasterok et al., 2019) may provide an alternative estimate of heat flow based largely on two well-constrained variables: surface and bedrock topography. However, it is dependent on the quality of constraints on crustal thickness, density, heat production, and thermophysical properties of the upper crust (of which uncertainty in upper-crustal heat production has the largest effect; Hasterok and Chapman, 2007b). For example, regions where high surface heat flow is dominantly from anomalously high upper-crustal heat production will have lower elevations than regions of similar surface heat flow but with lower upper-crustal heat production. Crust that has experienced tectonic and magmatic activity in the Cenozoic (i.e. <66 Ma) may be in a transient rather steady-state thermal regime, so this approach may have challenges in West Antarctica. Steady-state thermal modelling is thus more applicable to the old, stable crust of East Antarctica, particularly if the heat flow and isostasy of the conjugate margins are considered (Hasterok and Gard, 2016; Pollett et al., 2019). However, differences between the crustal thickness based on gravity modelling and isostatic elevation modelling may indicate variable densities and/or compositions of the underlying mantle (Pappa et al., 2019a, b).
4.6 Enhancement of GHF estimates by incorporation of heterogeneous crustal compositions
The geophysical approaches described above assume laterally homogenous heat production in the crust. However, given the geologically heterogeneous composition of the crust, it is important to consider the effects of variable lithospheric heat production and incorporate this into forward models of GHF.
Radiogenic heat production in the upper-crust contributes an estimated 26 %–40 % of the total continental GHF (Artemieva and Mooney, 2001; Hasterok and Chapman, 2007b, 2011; Pollack and Chapman, 1977; Vitorello and Pollack, 1980). Radioactive isotopes of the heat-producing elements (HPEs) uranium, thorium, and potassium (U, Th, and K) are responsible for ∼98 % of lithospheric heat production (Beardsmore and Cull, 2001). These elements are incompatible with mineral structures in the mantle and lower crust, so they concentrate in the upper crust and decrease in abundance with depth during planetary differentiation (the chemical and physical separation of an initially homogenous planetary body into one with an iron-rich core, magnesium-silicate-rich mantle, and a thin silicate-rich crust; Roy et al., 1968; Rudnick and Fountain, 1995).
The upper crust itself is highly heterogeneous in composition. HPE distribution is determined by their compatibility in different minerals, concentrating them in Si-rich silicic rocks (e.g. granite or rhyolite) relative to Fe-rich mafic rocks (e.g. gabbro or basalt). Immature sediments inherit the HPE abundance of their eroded source rocks but decrease in HPE abundance with increasing maturity and the consequent decrease in their lithic contents (Burton-Johnson et al., 2017; Rybach, 1986). Crustal heat production is thus heterogeneous, and the most significant control of HPE abundance and resultant heat production in the lithosphere is the distribution of the composite lithologies of the upper crust (Lachenbruch, 1968; Sandiford and McLaren, 2002; Taylor and McLennan, 1985).
4.6.1 Whole-rock geochemical analysis of heat production
Heat production of exposed lithologies can be determined from their concentrations of HPE (U, Th, and K) determined by geochemical analysis, or by airborne or ground-based gamma ray surveys. Radiogenic heat production for each sample (H, µW m−3) for the present day (t=0) can be determined from Eq. (7) (Turcotte and Schubert, 2014):
where , , and are the measured concentrations (ppm) of U, Th, and K respectively; HU238, HU235, HTh232, and HK40 are the heat productivities of the respective isotopes 238U ( Wkg−1), 235U ( Wkg−1), 232Th ( Wkg−1), and 40K ( Wkg−1), and D is the assumed density of the rock (e.g. 2800, 2850, and 3000 kg m−3 for felsic, intermediate, and mafic granulites respectively; Hasterok and Chapman, 2011). When using geochemical data to calculate heat production, this allows new and archive data to be used to calculate the heat production of the sampled outcrop. However, many archive analyses occurred prior to the development of accurate U quantification (e.g. by high-resolution X-ray fluorescence (XRF) or inductively coupled plasma mass spectrometry (ICP-MS)). An empirical relationship (Eq. 8; Burton-Johnson et al., 2017) allows calculation of total U, Th, and K heat production (H) from samples possessing only Th and K data (HK,Th; correlation coefficient, R2=0.9; Fig. 13).
Heat production values can be assigned to bedrock geology either by interpolation of the point values or by assigning the point values to the mapped geology and assigning their average value to the geological unit, the average being either the mean (Veikkolainen and Kukkonen, 2019), area-weighted mean (Slagstad, 2008), or median value (Burton-Johnson et al., 2017). Interpolation shows spatial variability within a unit but is affected by the interpolation method used, requires sufficient and evenly distributed data coverage, and is affected by anomalous values. For these reasons, the median values were used for the unevenly distributed archive data of the Antarctic Peninsula (Burton-Johnson et al., 2017). In Antarctica, maps of median (Antarctic Peninsula, Fig. 6; Burton-Johnson et al., 2017) and transects of mean (coastal East Antarctica; Carson et al., 2014; Carson and Pittard, 2012) heat production data have been integrated with geophysical models of the deeper heat flow to estimate the total GHF at the bedrock surface.
Integrating spatially variable upper-crustal heat production into the geophysical models of Antarctic GHF resulted in increased estimated spatial GHF variability, including local regions of high GHF above HPE-enriched granitic intrusions (Carson et al., 2014; Leat et al., 2018). The relative concentration of the HPE into the upper crust may result in it contributing a highly variable 6 %–70 % of the total GHF, although 3D crustal modelling is required to constrain its thickness (Burton-Johnson et al., 2017). This modelling also showed the impact of sedimentary basins on GHF distribution, as thick, extensive units of immature, clay-rich sediments may form extensive regions of enhanced GHF, even though more mature, quartz-rich sediments are associated with low GHF (Burton-Johnson et al., 2017). This highlights the importance of accurately constraining the upper-crustal geology and its chemistry when estimating GHF from geophysical data.
4.6.2 Glacially derived rock clasts
Although heat production can be determined for exposed bedrock, the likely heat production of the rocks beneath the Antarctic ice sheet is harder to constrain. To investigate East Antarctica, glacial clasts were sampled from moraines adjacent to the Transantarctic Mountains (Goodge, 2018). Granitic samples older than 500 Ma (Ross Orogen) were selected as likely lithologies of the interior of East Antarctica, as these are the dominant lithologies of other Precambrian cratons (>542 Ma regions of tectonically stable continental crust; e.g. central Canada). These clasts were analysed for their HPE abundance and attributed to their likely source area (the drainage basin of their associated glaciers). A probable range of subglacial heat flow values was estimated by assuming mantle and lower-crustal GHF values and a thickness for the upper crust based on other Precambrian shields. This indicates that East Antarctic heat flow is comparable to other Precambrian cratons and comparable to geophysical models of East Antarctic heat flow (Van Liefferinge and Pattyn, 2013). However, broader application of this approach is biased towards more erosion-resistant rock types, whilst less competent lithologies will not be preserved after glacial transport and deposition.
4.6.3 Gamma ray spectrometry
Rather than whole-rock geochemical analysis, the gamma ray spectrum can be used to determine the concentrations of radioactive isotopes, including those of K, Th, and U, and was first used for U exploration. Gamma ray spectrometry can be surveyed in the field, on samples, or from the air. Airborne surveys can cover large areas and have been used to survey Western Australia, SW England, and all of Finland (Beamish and Busby, 2016; Bodorkos et al., 2004; Hyvönen et al., 1972). However, the data require multiple corrections, and the recorded data integrate the radiation from the bedrock, surface cover (including soil and vegetation), atmosphere, cosmic radiation, and aircraft, making the data less accurate than ground measurements or sample analysis (Veikkolainen and Kukkonen, 2019). The technique is only sensitive to the upper 25 cm of the land surface, with overlying sediments and water bodies masking the radiation and leading to underestimates of heat production (Phaneuf and Mareschal, 2014). However, if the signal could be linked to mapped geological units and other evidence for subglacial geology (e.g. aeromagnetic and gravity anomalies), it may be feasible to extrapolate the calculated heat production beneath the ice sheet. Handheld gamma ray spectrometry studies, where heat production can be correlated with lithology along exhumed crustal profiles, show promise in this regard elsewhere (Alessio et al., 2018).
4.6.4 Crustal structure
Whilst surface HPE distribution can be constrained by measurements, the vertical distribution is more ambiguous. In heat flow models, heat production is often assumed to decrease exponentially with depth (e.g. Fox Maule et al., 2005; Martos et al., 2017). This exponential model was developed to explain observations from exposures of large, thick composite granite bodies (batholiths) where magma was initially emplaced at different depths in the crust (Lachenbruch, 1968, 1970; Swanberg, 1972) and reflects a proposed decrease in HPE abundance with increasing metamorphic grade (Lachenbruch, 1968; Sandiford and McLaren, 2002). However, this relationship has been challenged by other studies comparing HPE abundance and metamorphic grade (Alessio et al., 2018; Veikkolainen and Kukkonen, 2019), showing that the lithological change from the largely silicic upper crust to the mafic lower crust has a larger influence on HPE abundance than metamorphic grade (Bea, 2012; Bea and Montero, 1999). Deep (9–12 km) boreholes also show a correlation of heat production with lithology, but not with depth (Clauser et al., 1997; Popov et al., 1999). In fact, heat production increased for the first 2 km of the 12 km super-deep well of the Kola Peninsula, Russia, and then remained variable but high with increasing depth (Popov et al., 1999). Similarly, heat production increases below 3 km in the recent 5 km UD-1 well of the Cornubian batholith, UK (Dalby et al., 2020). As such, the available evidence indicates that the first-order HPE distribution is controlled by the HPE abundance of the crust prior to metamorphism and the vertical distribution of the crust's composite rock types. Inversely, it indicates that HPE distribution is not controlled by depth in the crust or the degree of metamorphism resulting from the increase in pressure and temperature.
Without evidence for the deeper structure of the crustal column, the lithological and HPE distribution of the lithosphere can instead be modelled as layers of variable thickness and heat production: the upper crust, middle crust, lower crust, and mantle lithosphere. Surface heat flow is largely insensitive to variations in the heat production or thickness of the mafic lower crust and mantle lithosphere due to their heat production being ∼1–2 orders of magnitude lower than that of the upper crust (Hasterok and Chapman, 2011; Rudnick and Fountain, 1995; Rudnick et al., 1998). The middle-crustal layer can either be excluded (Hasterok and Chapman, 2011) or be treated as a layer of invariable heat production (e.g. An et al., 2015b, for Antarctica) due to its low heat production compared with the range of the upper crust. Lithospheric heat production can thus be defined by the heat production and relative thickness of the upper crust, or upper-crustal heat-producing layer (Hasterok and Chapman, 2011). This can be defined by
where Qs is the surface heat flow, Qb is the basal heat flow of the upper crust, HUC is upper-crustal heat production, D is the thickness of the upper-crustal heat-producing layer, and F is the proportion of the surface heat flow contributed by the basal heat flow (Qb) (adapted from Hasterok and Chapman, 2011).
Rather than a simple layered model, more complex 2D or 3D models of upper-crustal structure can be developed using geophysical data, and the 2D or 3D crustal units assigned heat production and conductivity values based on analyses of representative exposures. A 3D crustal model derived from gravity and aeromagnetic data was developed to map heat flow in Norway (Ebbing et al., 2006; Olesen et al., 2007). In Antarctica, this has been applied in 2D to the high heat production granites of the Ellsworth–Whitmore Mountains using airborne magnetic and gravity data and bedrock topography (Leat et al., 2018) and the Transantarctic Mountains using topography and satellite gravity data (Pappa et al., 2019b).
Even though variability in deep lithospheric heat production has a smaller effect on surface heat flow than variability in upper-crustal heat production (Hasterok and Chapman, 2011), it is not homogenous. These thermophysical properties can be constrained from deep xenoliths (fragments of rock entrained in magma rising from depth) (Hasterok and Chapman, 2011; Martin et al., 2014) and crustal sections (Berg et al., 1989), which can also inform on the local geothermal gradient at the time of their crystallization.
To help constrain the properties of the Antarctic mantle, including its influence on Antarctic heat flow, a Geological Society of London memoir is currently being compiled summarizing the data gained from mantle xenoliths (Martin and van der Wal, 2020). This includes a sample database and a compilation of grain size and water content. These xenoliths are from shallow sources, as their occurrence is biased towards areas of crustal rifting where the lithosphere is thinner, although some xenoliths are from deeper sources (e.g. from the Amery Rift and Ferrar Dolerite).
Although geothermal heat flow has a geological derivation, it can also be constrained by multiple approaches through its observable effects on the overlying ice sheet. Inverse modelling can be applied to observed glaciological properties (e.g. glacial flow and melt rates), and the required GHF can be calculated. We will describe in this section different methods used in glaciology to derive GHF.
5.1 Subglacial water
The presence of subglacial water can be detected with an ice-penetrating radar. The reflective properties of the ice–bedrock interface depend on the presence of water, and, with certain caveats, radar surveys can be used to map subglacial water. In general terms, a glaciological model can then be used to estimate the values of GHF that better predict where basal temperatures reach the pressure melting point and melting occurs. We will describe in this section examples of this approach.
Carter et al. (2009) modelled the dielectric loss of radar data through the ice column around Dome C in East Antarctica (Fig. 6) to infer the basal reflectivity and verify the presence of subglacial water. Because the temperature profile of the ice sheet is one parameter affecting dielectric loss, this approach required inference of the basal heat flow from temperature–depth modelling over the last 254 kyr. The Shapiro and Ritzwoller (2004) GHF model was used initially (see Sect. 4.2), but when the calculated vertical ice velocity (mW) at the bed exceeded the initial melt rate (mT), the GHF was modified until mT and mW were equal. This approach identified localized high GHF anomalies, but (excepting these anomalies) they calculated that 66 % of the study area was either at or near the pressure melting point (anywhere that ice is thicker than 3500 m) without invoking enhanced GHF.
Schroeder et al. (2014) modelled the spatial distribution of melt beneath the ice sheet in the Thwaites Glacier catchment (Fig. 6) by mapping the relative bed echo strength of radar data in the region and modelling the water routing required to match these observations by routing alone (without heterogeneous basal melting). These routing models were based on the radar-derived ice thickness and surface slope. The 50 selected routing models were used to model the relative melt required to reproduce the observed echo strengths of each routing model. This relative melt model was in turn scaled to match the total meltwater produced in an ice sheet model of the Thwaites Glacier incorporating frictional melting, horizontal advection, and an assumed uniform GHF. By subtracting the frictional and advective contributions, the GHF required to produce the remaining melt could be calculated. This approach predicted very high heat flow in this region (114 to >200 mW m−2), with the highest heat flow focused around observed and inferred subglacial volcanoes.
With the aim of determining appropriate sites of low basal melting for old-ice drilling, Passalacqua et al. (2017) also used radar evidence for basal melting and ice sheet modelling to determine GHF around Dome C (Fig. 6). Wet and dry bed conditions were identified from radar data, and 10 spots were identified on bedrock topographic features marking the critical ice thickness where present basal melting becomes possible. These spots were defined as locations where the upper slopes of the bedrock topography are dry and their lee slopes are wet, with melting initiating between the two when the ice thickness passes the pressure melting point (Fig. 14). Assuming that GHF is locally homogeneous between the two bedrock elevations, heat flow was determined by increasing its value in a 1D heat model of the local ice thickness until basal melting occurred. These point estimates were interpolated to generate an approximate map of regional heat flow and calculate basal melt rates over the last 400 kyr.
Van Liefferinge and Pattyn (2013) and Van Liefferinge et al. (2018) used steady-state and transient thermodynamic modelling of the East Antarctic Ice Sheet to map the minimum heat flow required to raise the basal temperature above pressure melting point and generate basal melting. Whilst this was executed to identify possible sites for drilling the oldest ice in areas that are unlikely to have undergone basal melting in the last 1.5 Myr and did not produce an estimate of absolute GHF, if this approach were combined with other evidence for basal conditions above the pressure melting point (e.g. combining thermodynamic modelling with subglacial lake locations), points of minimum heat flow could be mapped.
5.2 Subglacial lakes
If temperatures are sufficient for basal melting, and topography depressions are suitable, subglacial lakes can develop. Subglacial lakes exhibit radio reflectivities 10–20 dB greater than the ice–bedrock boundary, allowing the current identification of at least 402 lakes beneath the Antarctic ice sheet (Wright and Siegert, 2012).
Whether basal temperatures are sufficient for basal melting and preservation of subglacial lakes is dependent on ice thickness, the surface temperature and accumulation rate, heat transported through ice advection, heat produced by internal deformation and basal sliding, and the GHF. When subglacial lakes are located near ice divides, heat derived by horizontal advection, basal friction, and internal deformation is assumed to be minimal, and thus the heat required to bring the base of the ice sheet above the pressure melting point is a product of ice thickness and GHF. Thus, when subglacial lakes are located near ice divides and the accumulation rate is known (high accumulation rates cool the ice mass), point estimates of minimum GHF can be calculated from one-dimensional thermal models of the ice sheet temperature profile (Van Liefferinge and Pattyn, 2013; Siegert, 2000). However, there is an assumption that water was derived locally and not routed from elsewhere (Passalacqua et al., 2017). Bedrock topography must also be considered as lakes can only form in topographic depressions. The absence of a lake or basal water does not imply the bed is frozen if the water can drain away (Pattyn, 2010; Siegert and Dowdeswell, 1996).
Conversely, and with the same caveats regarding basal topography and drainage, where the ice sheet is known to be frozen to the bed, the maximum GHF can be estimated. For example, Fudge et al. (2019) used the presence of Raymond Arches to deduce where the ice was frozen to the bed at the Siple Coast ice rises to estimate maximum GHF values. Combined, maximum and minimum estimates are more useful than either alone.
5.3 Englacial stratigraphy
Jordan et al. (2018) identified drawdown of internal ice sheet layers and increased bed reflectivity from radar data ∼200 km from the South Pole (Fig. 6), indicating enhanced basal melting. Melt rates were calculated using dated radar layers, traced from the Dome C ice-core site and a depth age model that simulates the drawdown effect of ice from subglacial melt rate. The low ice velocity (<1.5 m a−1) indicated minimal frictional contribution to basal temperature, and a location at the top of a hydraulic catchment area indicated a low heat contribution from subglacial water. By negating these contributions to heat flow, assuming the basal temperature is at the pressure melting point (and thus could be derived from the ice thickness) and that temporal temperature variations match those of the Dome C ice core, a time-dependent heat equation was applied to the ice sheet to derive the basal GHF required to generate the enhanced melt rates.
5.4 Microwave emissivity
Englacial temperature profiles have been derived from satellite and airborne passive detection of high-frequency L-band microwave radiation (∼1.4 GHz; Macelloni et al., 2019, 2016; Passalacqua et al., 2018), data primarily collected to investigate soil moisture and ocean salinity (Kerr et al., 2010). These wavelengths have very low absorption in ice and low scattering by particles (e.g. grain size and ice bubbles), providing high penetration depths in dry ice.
Macelloni et al. (2019) derived englacial temperature profiles for the Antarctic ice sheet from 2-year averaged vertical-polarized (V) radiation collected at the “Brewster angle” (; the angle of incidence at which the radiation is perfectly transmitted through the air–snow interface with no reflection, minimizing the influence of surface or shallow sub-surface effects). The corrected intensity (brightness temperature, TB) correlates with the surface temperature of the ice but is also affected by the ice sheet thickness (a largely inverse correlation), density profile, and grain size (Macelloni et al., 2016). As such, the ice sheet's thermal structure at depth could be estimated by comparing the observed TB and a simulated TB derived through microwave emissivity modelling, including one-dimensional modelling of the ice sheet's temperature profile. Included in the assumed values for this modelling are the GHF and the accumulation rate, the sources of greatest uncertainty. This method only applies in areas of slow-flowing ice (<10 m yr−1) and is optimal in areas of very slow-flowing ice (<5 m yr−1) as this negates heating by horizontal ice advection and deformation-derived heat production. It is also only applicable to areas of thick ice (>1000 m) as the simulations used to model microwave emission do not include bedrock reflections. This is not a limitation for application to Antarctic GHF research, as it is under these conditions that heat flow has the greatest influence on ice sheet dynamics.
Comparison of the microwave-derived temperature profile and that simulated by glaciological modelling (Van Liefferinge and Pattyn, 2013) show good agreement in the upper third of the ice sheet but diverge in their temperature estimates with depth, with the largest uncertainties close to the bedrock. This is largely due to uncertainty in the GHF but also reflects a decrease in sensitivity of the simulated TB to the temperature profile below 1000–1500 m (the bottom 1000–1500 m of the ice sheet contributes <10 % to the total emission). Longer wavelength emissions (0.5 GHz) with greater sensitivity to the deeper temperature profile may provide greater accuracy at depth (Jezek et al., 2014). Deep measurements of the ice sheet's temperature profile are required to validate this method compared to the glaciological models. Although currently limited by its sensitivity to temperature at depth and the accuracy of the assumed parameters (notably accumulation rate), this approach has the potential to constrain basal heat flow though variation in the assumed GHF values used in the emissivity modelling.
Although subglacial borehole-derived estimates of terrestrial GHF are lacking in Antarctica, estimates have been made from probes into marine sediments and boreholes into exposed bedrock. We have compiled 431 of these point estimates (Fig. 15; data available in the Supplement and from https://github.com/RicardaDziadek/Antarctic-GHF-DB, last access: 6 November 2020). The compiled data originate from multiple methods and are variable in their accuracy and limitations, and so we have attempted to qualitatively grade the likely reliability of each estimate based on specific parameters (Supplement). We do not include values for marine measurements compiled in the database “Global Heat Flow Data – Abbott Compilation”. This database is available via GeoMapApp and completely undocumented. The labels may point to cruise reports but not published data, and the data quality remains impossible to evaluate up to this point.
6.1 Boreholes into bedrock
Terrestrial, borehole-derived measurements of the geothermal gradient (12 boreholes, Supplement) are limited to the Dry Valleys and McMurdo Sound region (Fig. 15; Bucher, 1980; Decker, 1974; Decker and Bucher, 1982; Pruss et al., 1974; Talalay and Pyne, 2017), and no subglacial terrestrial borehole measurements have been made into the Antarctic bedrock. However, as discussed in Sect. 3.1, temperature gradients in bedrock must be taken to a sufficient depth to be representative of upward conduction of the GHF rather than downward conduction of the surface temperature. Whilst the GHF estimates from the Dry Valley Drilling Project (DVDP, including McMurdo Station) were taken from the 75 to >300 m deep boreholes (Bucher, 1980; Decker and Bucher, 1982; Talalay and Pyne, 2017), the shallow 7.6 m borehole from McMurdo Station produces a much higher GHF estimate (164 mW m−2; Risk and Hochstein, 1974). This shallow measurement should thus be neglected in preference for the 66 mW m−2 value from the 260 m deep DVDP borehole (Decker and Bucher, 1982).
Boreholes into submarine bedrock (34 boreholes, Supplement) have been drilled and temperature gradients measured beneath the McMurdo Sound, Amundsen Sea Embayment, and Ross Ice Shelf (Fig. 15; Bücker et al., 2001; Decker et al., 1975; Gohl et al., 2019; McKay et al., 2018; Morin et al., 2010).
The US Rapid Access Ice Drill project (RAID) aims to achieve the first subglacial, borehole-derived thermal measurements of bedrock following drilling of the overlying ice sheet and coring of ≥25 m of bedrock (Goodge and Severinghaus, 2016).
6.2 Ice boreholes
GHF estimates from ice boreholes (15 boreholes, Supplement) are better distributed across the Antarctic continent than terrestrial bedrock boreholes (Fig. 15). However, not all ice boreholes drilled have been sufficiently deep or in appropriate sites for GHF estimation (i.e. the ice sheet needs to be stationary and frozen to the bed). This limits the available GHF estimates to Vostok (Salamatin et al., 1998), Law Dome (Dahl-Jensen et al., 1999), South Pole (Price et al., 2002), Marie Byrd Land (Clow et al., 2012; Engelhardt, 2004; Gow et al., 1968), and the Antarctic Peninsula (Mulvaney et al., 2012; Nicholls and Paren, 1993; Zagorodnov et al., 2012) (Fig. 15). Dome Fuji (Hondoh et al., 2002) is not frozen to the bed but provides a minimum GHF estimate.
6.3 Marine and onshore unconsolidated sediments
The most abundant resource of heat flow estimates from measured temperature profiles around Antarctica comes from unconsolidated marine sediments (Fig. 15; 362 measurements south of −72∘ S, Supplement). However, the data distribution is sparse and heterogeneous, and whilst some regions are well sampled (e.g. the Amundsen Sea embayment; Dziadek et al., 2019, 2017), other regions (e.g. the Weddell Sea) remain poorly constrained (Fig. 15). In addition to the open water measurements, two shallow probes (deepest sensors at 1.4 and 0.8 m below the upper sediment surface) have measured the temperature gradient in subglacial sediments below the Whillans Ice Stream (Begeman et al., 2017; Fisher et al., 2015; see Sect. 3.3). Two temperature gradients have also been measured beneath the Ross Ice Shelf (Foster, 1978; Morin et al., 2010), but otherwise heat flow beneath the Antarctic ice shelves remains poorly constrained.
As discussed in Sect. 3.3, when using these estimates it is important to consider whether the shallow ( m) temperature gradient recorded by the probe is representative of the deeper GHF, or whether it has been perturbed by temperature variation in the overlying ice sheet or water column (e.g. Dziadek et al., 2019). Consequently, the water depth, the temperature profile of the water column, and possible sources of long-term temperature variation (e.g. variations in deep water circulation and temperature) should be considered when selecting appropriate point estimates. Similarly, whilst the shallow temperature gradients measured from subglacial Lake Whillans (Fisher et al., 2015) and the Whillans Ice Stream grounding zone (Begeman et al., 2017) are presented as subglacial direct measurements of Antarctic GHF, by the nature of their location within an ice stream they are not in a thermal steady state, and the temperature profile will have been affected by long-term variation from heat advection and shear heating. These are effects that cannot be evaluated from their very shallow temperature gradient (0.8 and 1.4 m deep), and accordingly these estimates should be used with caution.
The collated existing data and methodologies presented above highlight our current limitations in determining the subglacial GHF of Antarctica and allow discussion of future research.
7.1 Borehole- and probe-derived estimates
The fundamental limitation for GHF estimation in Antarctica is the lack of borehole-derived estimates from beneath the Antarctic ice sheet. Without these independent, discrete validation points, the more extensive regional estimates cannot be accurately evaluated. Therefore, the most promising future development will be the ≥25 m deep bedrock borehole measurements of the Rapid Access Ice Drill project (RAID; Goodge and Severinghaus, 2016). However, (as noted above) local temperature gradients may not be representative of the regional heat flow, as local geology, hydrothermal circulation, and topography can result in localized GHF variability. In response, multiple boreholes where the basal ice is frozen to the bedrock are required to categorize the regional variation, and topographic effects must be considered and accounted for. Topography may have significant effects on GHF via its effects on heat diffusion pathways to the surface (Bullard, 1938; Lees, 1910) and must be considered and investigated in GHF estimates at all scales, including those based on local temperature gradient measurements (i.e. borehole and probe-derived estimates) and more extensive geophysical and glaciologically derived models.
It is also a necessity that thermal modelling of the bedrock temperature profile for the RAID target sites is executed prior to drilling to constrain the penetration depth of low-frequency time variation in temperature. Whilst the RAID target bedrock borehole depth of ≥25 m is much shallower than the >100 m borehole depth achieved for exposed bedrock (Sect. 3.1), the overlying ice sheet insulates the bedrock temperature profile from short-duration surface temperature variability (temperature variation penetration depth is dependent on the frequency of the variation and thermal diffusivity of the material; Carslaw and Jaeger, 1959). However, as is considered for GHF estimates from ice boreholes (Sect. 3.2), low-frequency variation in surface temperatures, heat advection, and shear heating will all affect the subglacial temperature profile. Consequently, low-frequency temperature variation must be corrected for, and boreholes are best drilled where the ice is stationary and frozen to the bed (as is applied to ice borehole selection for GHF estimation). By drilling in such sites where glaciological approaches are most effective for GHF estimation, the RAID data will allow validation of GHF estimates for the various englacial temperature methods applied to stationary ice at ice divides (Sect. 5). These methods include borehole temperature profiles, subglacial lakes, ice sheet models, and microwave emissivity. It is thus important that the englacial temperature profile is measured in addition to the bedrock temperature gradient.
Beyond bedrock drilling there is lot to be gained from further ice borehole drilling. Firstly, existing data must be evaluated to ensure the methodologies of GHF modelling from borehole temperature profiles are consistent and accurate. Future ice boreholes into stationary ice frozen to the bed have the potential to supplement the existing borehole and probe-derived GHF estimates, particularly if the proposed methodology for shallow boreholes can be validated (600 m depth, or the upper 20 % of the ice column; Sect. 3.2).
7.2 Geophysical GHF estimates
Whilst only geophysical methods have provided continental-scale GHF estimates, their values and distribution vary greatly (Figs. 5, 16, and 17). Probability density functions show that whilst there is better agreement in East Antarctica (Fig. 17a), the seismically derived models estimate more variable and slightly higher GHF than the magnetically derived models. In West Antarctica the discrepancies between models are greater (Figs. 5g and 17b) even when using similar techniques (compare the empirical seismically derived estimates of Shapiro and Ritzwoller, 2002, and Shen et al., 2020, Fig. 17b). However, none of the models of West Antarctica reflect the GHF distribution of other better-constrained rift systems (Fig. 17c; Lucazeau, 2019), where much more heterogeneous distributions and a greater proportion of high GHF values (>150 mW m−2) are expected.
The fundamental question thus remains: does the West Antarctic Rift System (WARS) have elevated GHF? The magnetically derived model of Martos et al. (2017) estimates high GHF, but the most recent forward and empirically derived seismic models do not (An et al., 2015b; Shen et al., 2020; Fig. 5). If the seismic models are correct, then the high GHF estimates of the magnetic model reflect thinning of the magnetic crust, but GHF has subsequently reduced in the ∼90 Myr since the dominant phase of WARS crustal extension in the Cretaceous (∼105–95 Ma; Siddoway, 2008; as illustrated in Fig. 9b). If the magnetic model is correct, then GHF remains elevated in response to the younger 43–11 Ma Cenozoic phase of crustal extension (Granot and Dyment, 2018; e.g. Fig. 9a). Subglacial hydrological modelling (Schroeder et al., 2014) supports the high GHF estimates in the Thwaites Glacier region of the WARS. However, high-fidelity borehole estimates and better constraints on the nature of the geology, lithospheric architecture, and tectonic history of the WARS are required if we are to resolve the different estimates and use other locations as analogues for verifying the modelled GHF distribution.
To evaluate the accuracies of the different models, uncertainty estimates are required. Uncertainties of <10 mW m−2 for the majority of Antarctica were presented for the Curie depth GHF model of Martos et al. (2017). However, not only are the modelled values greatly different from those derived by seismic modelling (An et al., 2015b), the calculated Curie depth is also deeper than the seismically or gravitationally derived Moho depth for large areas of the continent (Fig. 10). Even though this can occur where metallic phases are present in cratonic mantle (Ferré et al., 2013; Sect. 4.1), this cannot explain the full distribution, nor are these occurrences likely to be this extensive. Without being critical of the model itself, it is reasonable to dispute the accuracy of the calculated uncertainties and suggest that although their calculation from the geophysical data may be logical, there may be a geological contribution to uncertainty (e.g. lithological variation in the lithosphere) that is not being considered. As GHF models are utilized by researchers in different fields to those publishing the models, they cannot be independently evaluated by the user, and so accuracy in published uncertainty values is arguably more important than the accuracy of the model itself. We recommend that future research (including geophysical, geological, glaciological, and borehole and probe-derived estimates) is careful in its presentation of uncertainty.
The largest limitations to existing geophysically derived GHF models are uncertainties in the structure, composition, heat production, and thermophysical properties of the unexposed crust, lithosphere, and underlying mantle. All current continental models assume the lithosphere to be laterally homogenous in its composition and thermophysical properties, and although seismic GHF models (e.g. An et al., 2015b) incorporate variable mantle temperatures, its composition is assumed to be homogenous. Geophysical GHF models assume that lithospheric heat production is focussed in the upper crust and is orders of magnitude greater than the deeper heat production of the middle and lower crust and the mantle. These models assume that lithospheric heat production either exponentially decreases with depth (e.g. the Curie depth models of Fox Maule et al., 2005; Martos et al., 2017; Purucker, 2012) or is concentrated within a laterally homogenous layer of variable depth and constant heat production (e.g. the seismic model of An et al., 2015a, and the thermal isostatic model for Australia of Hasterok and Gard, 2016). However, although the lower crust is enriched in mafic rocks (iron-rich rocks of high crystallization temperature, e.g. basalt) of low heat production, deep boreholes and crustal sections have shown that whilst there is a correlation between heat production and lithology in the upper crust, there is no such correlation with depth or metamorphic grade (Sect. 4.6.3). Similarly, the assumption of laterally homogenous heat production has been shown to be unreasonable for estimation of Antarctica's GHF, which (like all continents) has a laterally variable geology and associated concentration of HPEs (Burton-Johnson et al., 2017; Carson et al., 2014). The exponential decrease model of crustal heat production should thus be rejected, and attempts should be made to derive the depth and structure of crustal heat production.
The most promising approach to address the challenge of uncertainty in the contribution to GHF from the unexposed crust and deeper lithosphere is the derivation of a three-dimensional lithospheric structure model for Antarctica. This approach uses geophysical modelling integrating seismic, magnetic, and thermal isostatic evidence and integrating into the modelling the heat production, conductivity, and petrophysical properties of exposed lithologies and deeper crustal xenoliths or crustal sections. A similar model was developed for Norway (Ebbing et al., 2006; Olesen et al., 2007), and an Antarctic model would build upon recent 2D and 3D geophysically derived models (Leat et al., 2018; Pappa et al., 2019a, b). This requires an expanded database of the geochemistry of Antarctica's rock outcrops (particularly the HPEs). Beneath the Antarctic ice sheet, where the surface geology is unknown, the lithologies and probable heat production are best constrained by determining the probable heat production of each drainage basin based on its detrital clasts (e.g. Goodge, 2018).
The assumption of a homogenous mantle composition beneath East Antarctica is challenged by discrepancies between the Moho depth models derived by gravity and isostatic modelling (Pappa et al., 2019a, b), as this indicates variable lithospheric mantle densities, or deeper mantle effects on topography. A review of the available mantle xenoliths and mantle-derived basalt chemistry may be able to constrain the composition of the mantle beneath Antarctica, and thermal isostatic modelling may be able to identify these regions of anomalous mantle anomalies (as in the Australian study of Hasterok and Gard, 2016). If the seismic data for Antarctica are sufficient to determine crustal density, such a thermal isostatic model would provide an additional independent method to determine the depth of the upper-crustal heat-producing layer (Hasterok and Chapman, 2011) and evaluate the other GHF models.
Finally, it is important to compare Antarctica with its conjugate margins (e.g. Pollett et al., 2019), where GHF and crustal structure are better constrained. This provides constraints on the GHF along the margins of East Antarctica, as well as informing on the geology beneath the ice sheet.
Beyond individual geological and geophysical approaches, a further challenge is how best to integrate different models. Robust methods must be developed to incorporate datasets with different resolutions and uncertainty, including techniques already used by the broader data analysis community. For example, Rezvanbehbahani et al. (2017) applied a multivariate regression analysis to estimate heat flow in Greenland from sparse and variable geological and geophysical models and data.
7.3 Glaciological GHF estimates
Englacial temperatures are more sensitive to GHF in areas of the interior of Antarctica where basal sliding is negligible (Sect. 2.1) Out of all the methods discussed to derive GHF in the Antarctic interior, the most promising method is to derive GHF from englacial temperatures obtained from microwave emission (Sect. 5.4) at a longer wavelength (0.5 GHz) than that the currently available (∼1.4 GHz). The increase in wavelength will reduce the uncertainty in englacial temperatures below 1000–1500 m (Jezek et al., 2014). By improving the estimations of englacial temperature near the bed, this will reduce the role of ice flow modelling required to extrapolate temperature from the partial-depth data. Potentially, if near-the-bed englacial temperatures are known with sufficient precision, GHF could be derived as from borehole thermometry (Sect. 3.2). However, the longer-wavelength method requires the acquisition of currently unavailable satellite-derived data. The method is only applicable in areas of thick, very slow-flowing ice, and within this area only two ice boreholes exist for validation. Further validation of the technique to determine the origin of the differences between the temperature model derived from emissivity data and glaciological thermal modelling (Macelloni et al., 2019) and other spatially variable processes affecting microwave emissivity must also be considered (e.g. wind speed, accumulation rate, surface roughness, and density heterogeneities in the firn layer; Passalacqua et al., 2018).
Existing glaciological data, like subglacial water distribution or dated englacial layers, have been successfully used in estimating heat flow in regions of thick, slow-flowing ice near ice divides, where advection and shear heating are minimized. To extend these regional studies to continental scale, both data and models have to be improved. A significant challenge for radar-derived subglacial water distribution is our ability to discriminate between water at the bed versus contrasts in the geometric properties of ice sheet and bed (Schroeder et al., 2014). However the improvement in radar techniques and the combination with seismic surveys and direct access observations are our best chance to improve our observations of subglacial hydrology (Ashmore and Bingham, 2014).
The inventory of subglacial lakes (Wright and Siegert, 2012) is a better constrained and expanding dataset. Subglacial lakes can be detected also using satellite surface altimetry (Fricker et al., 2007), providing a way to expand the coverage and to confirm dubious cases. However, as noted in Sect. 5.1, topography must be considered when using evidence for subglacial lakes as they can only develop in topographic depressions, and the absence of basal water does not imply the bed is frozen if water can drain away.
Subglacial melting can also be detected in englacial stratigraphy (Sect. 5.3) but the required radar product (internal radar reflective horizons) is not often available. “AntArchitecture” is a SCAR (Scientific Committee on Antarctic Research) Action Group bringing together key datasets on Antarctic internal layering from the principal institutions and scientists who have been responsible for acquiring, processing, and storing them over the last 4 decades (AntArchitecture Action Group, 2017). As the coverage of Antarctic internal layers becomes widely available, its application to infer GHF will increase in popularity.
Finally, and for any of the glaciological methods described above, the glaciological models used to infer GHF have to be improved. The current thermal models used to infer GHF can be classified in two larger groups: (1) 1D time-dependent high-complexity models and (2) 2D/3D steady-state low-complexity models. The first category is generally used near ice domes or ridges, with low horizontal flow, and where horizontal heat advection can be neglected (e.g. Passalacqua et al., 2017). The latter are used across the whole continent (e.g. Van Liefferinge et al., 2018), but they ignore the changes in temperature between glacial and interglacial periods despite their strong effect on englacial temperatures (Ritz, 1989). The challenge is to develop thermal models with the required level of complexity at a continental scale, accommodating the main physical processes. This remains a technical challenge, and thermodynamic models remain dependant on GHF estimates.
We present state-of-the-art data and models to estimate geothermal heat flow in Antarctica and highlight the need for a detailed continental map. We also discuss current challenges and future directions.
With multiple methodologies and models for Antarctic GHF currently published, the most promising future direction for local estimates is borehole-derived estimation of GHF beneath the Antarctic ice sheet from RAID bedrock drilling and englacial temperatures from ice boreholes. Ideally, the latter approach will be validated by the former to support expansion of the dataset from shallow boreholes (potentially only 600 m deep, or 20 % of the total ice sheet thickness).
The ice sheet is most sensitive to variation in GHF within the interior of Antarctica, where heat production from sliding at the base of the ice sheet is negligible. However, it is in this region that GHF is hardest to constrain by geophysical estimates because is of the scarcity of local GHF estimates from down-hole-measured temperature gradients, geological data, and insight from conjugate margins. It is thus in the interior of Antarctica where glaciological approaches are the most applicable. Out of the methods presented, the determination of englacial temperatures from long-wavelength microwave emissivity is the most promising, but these data are not currently available and require further validation.
We highlight the potential of regional estimates of GHF from subglacial meltwater inventories. Aside from the ever expanding inventory of subglacial lakes, we encourage initiatives like “AntArchitecture” that will make radar products widely available. Also, we discuss future requirements of thermal models (either 1D or those lacking glacial–interglacial variability) to expand the methods beyond domes in the interior of Antarctica.
Geophysical methods remain the most attractive approach to estimate GHF because they are independent of ice flow. However, they vary greatly in their estimated magnitude and distribution of GHF. The greatest uncertainty in all the geophysical models is uncertainty in the composition and structure of the lithosphere and mantle. We recommend ceasing to use the exponential decrease model of crustal heat production. Instead, we suggest using geological and geophysical approaches to model the thickness, structure, and composition of the crust. We also recommend the application of a thermal isostatic approach to provide an independent estimate and highlight regions of anomalous isostatic elevation and probable mantle heterogeneities. The effects of topography must also be considered in all GHF models.
Finally, the greatest challenge for Antarctic GHF estimation is the necessity of multidisciplinary science and how best to integrate the different methods. Hopefully this paper provides a first step in communicating the approaches and limitations of the different fields across the GHF community. We sincerely recommend the continuation and enhancement of the international collaborations within SCAR, building on the work of the GHF sub-group of the SERCE research programme (Solid Earth Response and influence on Cryospheric Evolution), and we encourage and appreciate SCAR's continuing support in this field of research.
The database of GHF point estimates (Fig. 15) is available in the Supplement and from https://github.com/RicardaDziadek/Antarctic-GHF-DB (last access: 6 November 2020, Dziadek and Burton-Johnson, 2020). The GHF mean and standard deviation maps of the geophysical models of continental GHF (Fig. 5f and g) are available in the Supplement.
The supplement related to this article is available online at: https://doi.org/10.5194/tc-14-3843-2020-supplement.
ABJ and RD conceived the project. ABJ was the lead author for all sections and the specialist in geology and geochemistry. RD was a co-author for all sections, compiler of the supplemental GHF database, and the specialist in geophysics. CM was a co-author for all sections and the specialist in glaciology.
The authors declare that they have no conflict of interest.
The authors thank Brice Van Liefferinge, the anonymous reviewer, and John Goodge for their helpful and thorough reviews and comments, which have all improved this final paper; Alexander Robinson for his work and comments as our handling editor; and the Copernicus team for all their assistance. This research is a contribution to the SCAR SERCE scientific research programme, and we thank the discussions and support of this group from the TACtical 2018 (Hobart, Australia), POLAR 2018 (Davos, Switzerland), ISAES 2019 (Incheon, Korea), and SCAR 2020 Open Science Conference (online) meetings. We particularly thank Jacqueline Halpin (IMAS, Hobart) for her comments on the manuscript and her work promoting and developing the Antarctic GHF community.
Alex Burton-Johnson and Carlos Martin were funded by the Natural Environment Research Council as part of the British Antarctic Survey Polar Science for Planet Earth programme. Ricarda Dziadek was supported by the Deutsche Forschungsgemeinschaft (DFG) in the framework of the Priority Program 1158 “Antarctic research with comparative investigations in Arctic ice areas” by grant GO 724/14-1. Additional funds were contributed by the AWI Research Program PACES-II Workpackage 3.2.
This paper was edited by Alexander Robinson and reviewed by Brice Van Liefferinge and one anonymous referee.
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