Gruber 2012 a Global View on Permafrost in Steep Bedrock

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    A Global View on Permafrost in Steep Bedrock

    Stephan Gruber

    Department of Geography, University of Zurich, Switzerland

    Abstract

    Mountainous topography covers a considerable proportion of the global permafrost region. There, temperature changes

    and the degradation of permafrost in steep bedrock can evoke rapid geomorphic change, some of which may result innatural hazards. Due to the strong relief of most rock walls, corresponding events can have a long runout and transform

    into cascading events, such as impact to lakes or the damming of rivers that propagate far below the periglacial zone. The

    identication of areas that potentially have permafrost conditions in steep rock is the important rst step in the evaluation

    of corresponding hazards. During the past decade, researchers have given considerable attention to permafrost in steep

    bedrock, although most investigations have been conducted in the European Alps. This contribution provides a summary

    of ndings related to the delineation of permafrost in rock walls. Based on this, simple considerations and data sources are

    outlined that may help the application of current knowledge in remote mountain regions.

    Keywords:bedrock slopes; mountains; steep terrain; global; hazard zonation; mapping.

    Introduction

    A signicant proportion of the global permafrost region

    has mountainous topography (Gruber 2011a). Additionally,

    coastal cliffs may be subject to permafrost conditions, and

    changes to permafrost there can alter the stability of rock

    faces perched high above valleys and thus pose a hazard to

    human life and infrastructure (cf. Carey 2005). This may

    occur indirectly through, for example, impacts to lakes that

    may cause long-distance secondary events (cf. Geertsema &

    Cruden 2008, Geertsema & Clague 2011). However, non-

    stationarity, incomplete understanding of processes, and lack

    of information on local surface and subsurface conditions

    challenge corresponding hazard zonation. Here, the delineation

    of permafrost rock slopes can serve as a proxy for areas thatmay require special attention or surveillance, as they are

    prone to rapid changes in response to climate forcing (Gruber

    2011b). Absent or minimal vegetation, a reduced snow cover,

    and less important active-layer processes make permafrost in

    steep rock a system that is simple enough for attempting an

    extrapolation of ndings to environments not measured. In this

    contribution, I summarize ndings on the spatial and temporal

    variability of mean annual ground temperature (MAGT) and

    permafrost in steep bedrock. These ndings, often based on a

    narrow range of environmental conditions, are extended with

    hypotheses for generalization to other environments. This is

    intended to support the estimation of permafrost conditions in

    steep rock globally, and to provide a framework to test andimprove them by means of measurement, experiment, and

    observation. Unless stated otherwise, the investigations cited

    have been performed in the European Alps.

    Rock Temperature: Factors and Processes

    Basic considerations

    The energy uxes at and near the ground surface are shown

    for the two conceptual end members of steep and homogenous

    bedrock and a horizontal debris slope in Figure 1. Longwave

    radiation is mostly affected by air temperature, moisture

    content, and clouds. Turbulent uxes mostly depend on airtemperature and wind.

    Solar irradiation, however, is strongly dependent on

    cloudiness, sun-terrain geometry, and topography, and results

    in a high degree of spatial differentiation. Figure 2 shows three

    conceptual scales that determine ground temperatures. When

    considering global patterns, differing climate conditions affect

    the strength of the topographic inuence.

    For example, in areas with more abundant clouds and diffuse

    radiation, topographic differentiation is less pronounced than

    in areas with few clouds and strong direct solar radiation. The

    Figure 1. Schematic of energy balance at and near the ground

    surface in steep bedrock (A) and gentle debris slopes (B).

    Figure 2. Conceptual scales of inuence on ground temperatures.

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    spatial differentiation of MAGT can be conveniently described

    relative to mean annual air temperature (MAAT) using

    (1)

    Because MAAT is a commonly available climate variable,

    dT helps to estimate local patterns relative to it. MAAT is

    often subject to strong intra-annual variation, but dT for near-

    vertical rock remains rather constant (cf. Noetzli & VonderMuehll 2010).

    Near-vertical and compact rock

    Near-vertical and compact rock faces exhibit a strong

    topographic control on subsurface temperatures and a weak

    thermal inuence of snow and active-layer processes typical

    for debris-covered slopes (Fig. 1). Spatial patterns of dT are

    dominated by direct solar radiation (cf. Hoelzle 1994) and

    modied by rock albedo (cf. Hall 1997). For this reason,

    they are a simple system to investigate and to then gradually

    expand by considering additional processes. Gruber et al.

    (2003) present a review of previous investigations and a

    strategy for measuring in steep rock faces. Corresponding data

    are available through PERMOS (cf. Noetzli & Vonder Muehll

    2010) and a pan-Alpine inventory of permafrost evidence

    (Cremonese et al. 2011). In near-vertical and compact rock,

    MAGT is often measured 530 cm below the surface and

    presumed to be equivalent to that just below the active layer.

    Based on the work of Allen et al. (2009) summarizing 14

    one-year time series from the Southern Alps of New Zealand

    (44S), dT in sun-exposed slopes can be estimated to 4.5

    6.5C. In the European Alps (46N), Boeckli et al. (2012)

    estimated this to be 5.56C based on 57 locations and a

    statistical model. A process-based modeling study (Gruber

    et al. 2004) in the European Alps resulted in dT rangingfrom 6.5 to 9C. The model is driven by daily data that do

    not resolve temperature differences between east and west

    exposure. This may result from convective clouding in the

    afternoon lowering the temperature on west-exposed faces by

    reducing direct solar radiation. Generally, dT increases with

    elevation due to more shortwave and less longwave radiation,

    and with decreasing precipitation due to a higher amount of

    direct radiation. Reection from surrounding snow-covered

    slopes can locally increase shortwave irradiation and thus dT.

    This effect is assumed to have affected dT at two measured

    locations by 23C (cf. Allen et al. 2009). Without any solar

    radiation, dT would become slightly negative due to longwave

    loss.Summarizing this paragraph, dT likely ranges from 0 to 9C

    in steep and compact rock at latitudes near 45, and varies

    mostly as a function of solar radiation.

    Surface heterogeneity and clefts

    Most rock slopes differ from the near-vertical case because

    micro-topography and fracturing promote patchy covers of

    debris, snow, and ice (Gruber & Haeberli 2007). The thermal

    inuence of snow, fractures, and active-layer processes can

    thus contribute to the heterogeneity of dT. Safety issues

    and the dominance of lateral heterogeneity in near-surface

    measurements of MAGT, however, complicate corresponding

    research. Gubler et al. (2011) found that MAGT on more

    gentle slopes can already vary by up to 2.5C within an area of

    10 m x 10 m. For heterogeneous bedrock slopes, this value is

    likely often exceeded.

    Using measurements at four depths down to 85 cm in

    borings and deeper on thermistor strings lowered into clefts,

    Hasler et al. (2011) estimated a local cooling effect of fractureson the order of 1.5C. This cooling resulting from ventilation

    likely depends on cleft aperture and abundance, and its

    functioning may resemble ventilation effects in coarse blocks

    (cf. Harris & Pedersen 1998) or, in extreme cases, those in

    ice caves (Obleitner & Sptl 2011, Schner et al. 2011). A

    local lowering of dT by several C, even in shaded slopes,

    thus appears possible in rare cases. For practical use, however,

    an assumption of 12C cooling, increasing from shaded to

    sun-exposed slopes, appears plausible for heterogeneous

    conditions. Snow deposited in clefts may have an additional

    cooling effect by consuming latent heat during melting. At

    the same time, however, snow cover or inll can inhibit air

    circulation and thus reduce the associated cooling (Hasler et

    al. 2011). A thermal diode effect caused by seasonally varying

    proportions of ice/water/air in pores and fractures can cause a

    lowering of temperatures at depth (Gruber & Haeberli 2007)

    similar to the thermal offset described for lowland permafrost

    (cf. Smith & Riseborough 2002), but this has not been detected

    in measurements (Hasler et al. 2011).

    Snow and perennial ice

    Snow on rock faces alters the coupling between the

    atmosphere and subsurface and thus affects dT. It is usually

    thinner and spatially and temporally more variable than in

    gentle terrain. Due to difcult access, corresponding studiesare rare (cf. Wirz et al. 2011). Rock faces often extend far

    above the equilibrium line of glaciers and receive much of their

    precipitation in solid form. In those conditions, temperature

    moderates the retention of snow because cohesive snow near

    melting conditions is more likely to accumulate than cold

    snow that is prone to be removed by wind and sliding. For

    cold and shaded faces, this can cause a pronounced snow

    cover during summer, whereas precipitation in winter barely

    affects the bare and dark surfaces of ice and rock (cf. Gruber &

    Haeberli 2007). Depending on the seasonality of precipitation,

    snow during summer can be common in high-elevation

    rock faces. For thin snow, the net warming through thermal

    insulation during winter is reduced and the relative importanceof cooling through albedo and latent heat uptake during melt

    becomes greater. Higher albedo decreases dT more strongly

    on sun-exposed slopes, whereas the effect of latent heat can

    cause a lowering of dT in all slope aspects.

    Based on numerical experiments under the assumption of

    laterally homogeneous snow cover, Pogliotti (2011) estimated

    this cooling to have magnitudes of up to 2C with respect to

    snow-free rock. In reality, this is further modied in laterally

    heterogeneous and discontinuous snow cover because a lateral

    interaction between snow-covered and snow-free rock facets

    dT= MAGT- MAAT

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    exists by heat conduction in rock as well as by radiative and

    sensible exchange at the surface (cf. Neumann & Marsh 1998).

    Based on distributed measurements of rock temperature,

    Hasler et al. (2011) estimated the cooling effect of snow in

    radiation-exposed faces to be up to 23C.

    Ice faces, hanging glaciers, or surface lowering of glaciers

    can inuence the temperature regime in steep rock and can

    exhibit strong spatio-temporal variations (Fischer et al.

    2011). While ice faces and hanging glaciers are diagnostic ofpermafrost conditions at their rock-ice interface, their absence

    does not indicate the absence of permafrost. The occurrence of

    cold rn (Suter et al. 2001, Suter & Hoelzle 2002, Hoelzle et

    al. 2011), and thus hanging glaciers, follows differing patterns

    than rock temperature because they are subject to higher albedo

    and are affected by wind through snow transport. In gently

    inclined parts of hanging glaciers, the percolation of water into

    the rn and heat release at depth during refreezing can cause

    zones of temperate rn and ice (Haeberli & Alean 1985). As

    a consequence, an inference of temperature below ice cover

    is difcult. For ice faces that are subject to minimal ow and

    balance change, a cooling with respect to rock is likely for

    sun-exposed slopes due to the inuence of albedo. For a north-

    exposed ice face, Hasler et al. (2011) report approximately the

    same mean annual temperature as in nearby rock.

    Three-dimensional and transient effects

    Spatial variation of surface conditions and their temporal

    changes inuence permafrost bodies at depth (cf. Gold &

    Lachenbruch 1973), and in mountain areas this is further

    complicated by geometric effects (Kohl 1999, Gruber et al.

    2004). The combination of a distributed MAGT model and

    three-dimensional heat-transfer modeling of steep topography

    (Noetzli et al. 2007) showed complicated permafrost bodies

    with steeply inclined isotherms near peaks and ridges. Even insteady-state, permafrost can be induced below non-permafrost

    terrain facets due to nearby cold slopes. Transient simulations

    were performed with a similar setup (Noetzli & Gruber 2009)

    and accounted for temperature changes during the past. This

    revealed the importance of past climate and latent heat that

    can lead to permafrost bodies persisting at depth below slopes

    that today would be interpreted as permafrost-free. Because

    of multi-lateral warming, the reaction of convex topography,

    such as ridges or rock spurs, can be much faster than that of

    at terrain (Noetzli & Gruber 2009). Several new boreholes

    in steep rock and in ridges (Noetzli et al. 2010, Noetzli et al.

    2008, Noetzli & Vonder Muehll 2010) support many of the

    general ndings from the modeling studies.

    The Global View: Estimating Spatial Patterns

    of Rock Temperatures for Diverse Mountain

    Ranges

    In this section, simple approaches for estimating permafrost

    occurrence in rock faces worldwide are proposed. It is

    important to keep in mind that this is based on limited point

    data from a restricted range of environmental conditions.

    Furthermore, the derivation of such heuristics has an element

    of subjectivity, especially where it involves the delineation of

    permafrost zones.

    Global distribution

    For strongly shaded rock faces, the 0C long-term isotherm

    of the MAAT is a good pointer to determine the elevation

    above which permafrost must be expected, even though

    permafrost may sometimes be found at lower elevation. Due

    to the absence of better data, the zonation shown in Gruber

    (2011a) can provide an approximation globally at about 1 km

    resolution. While few rock faces are dominated by inversion

    effects, inversions are important to consider in the choice

    of local meteorological stations as possible alternatives.

    As the extrapolation of MAAT in rugged terrain involvesconsiderable vertical distances, the choice of appropriate lapse

    rates is important. If suitable ground measurements do not

    exist, the lapse rate can be approximated based on model data

    (Gruber 2011a) or regional radiosonde measurements. MAAT

    data covering a period of several decades helps to minimize

    the inuence of short-term uctuations. It is sometimes

    necessary to account for longer-term transient effects that have

    occurred during the past decades or centuries with respect to

    the measurement period chosen (cf. Noetzli & Gruber 2009).

    Topography and solar radiation

    Topography inuences dT for individual slopes, mainly

    through its geometric effect on incoming solar radiation.Generally, steeper and more rugged terrain causes a wider

    range of dT than more gentle terrain. This effect, however,

    is modied by latitude and the proportion of direct radiation.

    As a rst approximation, a ruggedness index (e.g., Gruber

    2011a) can be used to identify terrain tending to have a higher

    proportion of steep and strongly shaded rock slopes. Locally,

    the differentiation of slopes with respect to solar radiation can

    be estimated based on the calculation of mean annual potential

    solar irradiation and a decameter-resolution DEM (e.g., Farr et

    al. 2007). This operation is routinely available in GIS software.

    Figure 3. Latitude-dependency of maximum (solid) and minimum

    (dashed) potential direct solar radiation received in rugged terrain.

    The experiment shown spans slope angles 090, slope expositions

    0180 (because east and west are identical in this respect), and has

    no horizon shading.

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    Latitude

    Besides its effect on MAAT, latitude inuences the

    maximum amount of total annual solar irradiation received by

    the most suitably exposed slope. For this reason, the range of

    dT is also likely to be affected by latitude (Fig. 3). Further,

    the partitioning of radiation with topography changes with

    latitude. Toward the poles, increasingly steep slopes receive

    the highest amounts of radiation; near the tropics, rather gentleslopes receive the highest radiation input. Furthermore, the

    sensitivity to cast shadowing by obstructed horizons increases

    toward the poles with the prevalence of low solar elevation

    angles.

    Continentality

    Continental (as opposed to maritime) climate is

    characterized by comparably large seasonal thermal variations

    and dryness, both generally caused by large distances from

    major water bodies and altered by atmospheric circulation

    patterns and rain-shadow effects. The dryness in continental

    areas is usually accompanied by very high amounts of direct

    solar radiation afforded by often cloud-free skies. BesidesMAAT, continentality is often used to describe spatial patterns

    of cryosphere phenomena (e.g. Holmlund & Schneider 1997,

    King 1986, Haeberli & Burn 2002, Shumskii 1964) and is

    frequently characterized by a continentality index dened as

    the average difference between the coldest and warmest month

    at a location.

    The continentality index shown in Figure 4 provides an

    appreciation of its global patterns that may help to inform the

    extrapolation of ndings from one mountain range to another.

    The patterns of temperature range, the proportion of direct

    sunlight, and precipitation are jointly described by the concept

    of continentality. However, these affect rock temperature in

    differing ways and often correlate much less than expected

    when plotted based on gridded climate data. Until further

    analyses help to disentangle these effects, the assumption of

    subdued spatial differentiation of dT toward maritime areas

    likely provides a good assumption. This effect of continentally

    or precipitation on the degree of spatial differentiation due tosolar radiation is, however, not clearly detectable in current

    measurements (cf. Allen et al. 2009, Boeckli et al. 2012) that

    span only small gradients.

    Surface characteristics

    As a general rule, rough surfaces can be assumed to be colder

    than smooth ones. Cooling is caused by a thin, intermittent,

    and frequent snow cover and by air circulation in fractures or

    debris.

    At least qualitatively, the roughness of rock walls can be

    assessed based on eld visits, photographs, aerial photographs,

    or high-resolution satellite imagery. Increasingly, the imagery

    freely available on GoogleEarth, for example, has sufcientresolution to provide valuable rst impressions.

    Conclusion

    Based on research from a narrow range of environmental

    conditions and the consideration of what appear to be the

    processes that govern permafrost distribution in steep bedrock,

    I have proposed simple considerations to estimate permafrost

    in rock walls worldwide. Besides the potential for practical

    application, this contribution points to the wide range of

    Figure 4. Continentality index derived from 20002010 mean monthly surface air temperatures based on ERA-Interim re-analysis data. Dark

    areas are maritime; light areas are continental climate.

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    environmental conditions that drive permafrost in steep terrain.

    More systematic research in integrating local and regional

    research to achieve a coherent understanding would be a good

    avenue to progress beyond the heuristics presented here. Such

    research would consolidate understanding by basing it on a

    wider range of environmental conditions.

    Acknowledgments

    Over the past ten years, many colleagues and friends

    have contributed toward the synthesis presented here.

    These contributions have come not only through the works

    referenced, but also though inspiring discussions and eld

    campaigns. Among these are: Jeannette Ntzli, Andreas

    Hasler, Marco Peter, Adrian Zgraggen, Lorenz Bckli, Jan

    Beutel, Simon Allen, Martin Hoelzle, Ludovic Ravanel, Paolo

    Pogliotti, Umberto Morra di Cella, Edoardo Cremonese, and

    Reynald Delaloye. ECMWF ERA-Interim data used in this

    study have been obtained from the ECMWF data server.

    Michael Krautblatter is acknowledged for valuable and

    insightful reviewer comments.

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