scholarly journals Helicopter-borne transient electromagnetics in high-latitude environments: An application in the McMurdo Dry Valleys, Antarctica

Geophysics ◽  
2016 ◽  
Vol 81 (1) ◽  
pp. WA87-WA99 ◽  
Author(s):  
Neil Foley ◽  
Slawek Tulaczyk ◽  
Esben Auken ◽  
Cyril Schamper ◽  
Hilary Dugan ◽  
...  

The McMurdo Dry Valleys are a polar desert in coastal Antarctica, where glaciers, permafrost, ice-covered lakes, and ephemeral summer streams coexist. Liquid water is found at the surface only in lakes and in the temporary streams that feed them. Past geophysical exploration has yielded ambiguous results regarding the presence of subsurface water. In 2011, we used a helicopter-borne, time-domain electromagnetic (TDEM) sensor to map resistivity in the subsurface across the Dry Valleys. The airborne electromagnetic (AEM) method excels at finding subsurface liquid water in polar deserts, where water remains liquid under cold conditions if it is sufficiently saline, and therefore electrically conductive. Over the course of 26 h of helicopter time, we covered large portions of the Dry Valleys and vastly increased our geophysical understanding of the subsurface, particularly with respect to water. Our data show extensive subsurface low-resistivity layers approximately 150–250 m below the surface and beneath higher resistivity layers. We interpret the low-resistivity layers as geologic materials containing freeze-concentrated or “cryoconcentrated” hyper saline brines lying beneath glaciers and frozen permafrost. These brines appeared to be contiguous with surface lakes, subglacial regions, and the Ross Sea, which could indicate a regional-hydrogeologic system, wherein solutes might be transported between surface reservoirs by ionic diffusion and subsurface flow. The presence of such brines underneath glaciers might have implications for glacier movement. Systems such as this, where brines exist beneath glacial ice and frozen permafrost, may exist elsewhere in coastal Antarctica; AEM resistivity is an ideal tool to find and survey them. Our application of TDEM demonstrates that in polar subsurface environments containing conductive brines, such a diffusive electromagnetic method is superior to radar surveying in terms of depth of penetration and ability to differentiate hydrogeologic conditions.

2021 ◽  
Author(s):  
◽  
Cassandra Anh Trinh-Le

<p>The hyper-arid, cryotic, wind-dominated conditions in the high-elevation McMurdo Dry Valleys of Antarctica are among Earth’s most extreme environments and represent the closest terrestrial analog to the surface of Mars. These unique conditions result in complex surface processes that occur in the overall absence of liquid water. However, since water is typically believed to be required for these processes to occur, the mechanisms responsible for how these processes can persist in this environment are poorly understood. Previous studies that focused on individual processes of sedimentation in the Dry Valleys leave questions regarding the role of water in dry cryotic sedimentation as well as the rates at which these processes occur. This thesis addresses these questions by combining Optically Stimulated Luminescence (OSL) dating, meteoric Beryllium-10 (10Be) measurements, soil geochemistry analysis, and petrographic microscopy analysis on ice-cemented permafrost cores taken from University Valley, one of the high-elevation Dry Valleys, where the availability and effects of liquid water are minimal. These analyses were used to explore four main sedimentation processes that occur in the Dry Valleys: chemical weathering, fine particle translocation, eolian transport, and physical weathering. Analyzed together, findings from these analyses comprehensively describe the complex processes involved in dry cryotic sedimentation and determine the roles of different phases of water in this environment.   Sediments in University Valley have accumulated at a rate of approximately 2.1 mm/ka for the last 200 ka, as dated by OSL, from erosion of the valley walls and deposition of windblown dust. Sediment accumulation is influenced by topography of the valley floor, depth of the ice table, aspect of the valley walls, wind direction, and mechanical breakdown of rocks due to solar heating. While persistent winds constantly remobilize fine particles and dust in the upper few cm of the dry ground, sediment grains that are sand-sized or larger do not undergo significant remobilization, and sediments in the ice-cemented ground are unaffected by remobilization and translocation processes. Rare clay bridges seen in thin section show that small, infrequent, transient surface wetting events have occurred over the last 200 ka. High anion concentrations associated with high surface meteoric 10Be measurements and clay bridges indicate that the source of these wetting events is the melting of wind-blown snow from coastal regions. Patterns in meteoric Be measurements show that these small transient wetting events are not sufficient to translocate fine particles through the soil profile, which suggests that the role of liquid water as a transporting agent is negligible in this environment. Chemical weathering in University Valley appears to be controlled by two main components: dolerite content of the sediments, and exposure to the atmosphere at the ground surface where condensation of water vapor onto grain surfaces readily leaches ions from dolerite grains under the oxidizing conditions of the Dry Valleys. In the absence of liquid water, chemical processes that occur in this environment rely on water vapor.   Together, these results indicate that surfaces in University Valley are remarkably young and sedimentologically active. Because University Valley represents one of the closest terrestrial analogs to the surface of Mars, findings from this thesis may be applicable to understanding the timescales and the processes that control anhydrous sedimentation on the surface of Mars.</p>


2008 ◽  
Vol 20 (5) ◽  
pp. 499-509 ◽  
Author(s):  
Peter T. Doran ◽  
Christopher P. McKay ◽  
Andrew G. Fountain ◽  
Thomas Nylen ◽  
Diane M. McKnight ◽  
...  

AbstractThe meteorological characteristics and hydrological response of an extreme warm, and cold summer in the McMurdo Dry Valleys are compared. The driver behind the warmer summer conditions was the occurrence of down-valley winds, which were not present during the colder summer. Occurrence of the summer down-valley winds coincided with lower than typical mean sea level pressure in the Ross Sea region. There was no significant difference in the amount of solar radiation received during the two summers. Compared to the cold summer, glaciological and hydrological response to the warm summer in Taylor Valley included significant glacier mass loss, and 3- to nearly 6000-fold increase in annual streamflow. Lake levels decreased slightly during the cold summer, and increased between 0.54 and 1.01 m during the warm summer, effectively erasing the prior 14 years of lake level lowering in a period of three months. Lake level rise during the warm summer was shown to be strongly associated with and increase in degree days above freezing at higher elevations. We suggest that strong summer down-valley winds may have been responsible for the generation of large glacial lakes during the Last Glacial Maximum when ice core records recorded annual temperatures significantly colder than present.


2010 ◽  
Vol 23 (13) ◽  
pp. 3577-3598 ◽  
Author(s):  
Johanna C. Speirs ◽  
Daniel F. Steinhoff ◽  
Hamish A. McGowan ◽  
David H. Bromwich ◽  
Andrew J. Monaghan

Abstract Foehn winds resulting from topographic modification of airflow in the lee of mountain barriers are frequently experienced in the McMurdo Dry Valleys (MDVs) of Antarctica. Strong foehn winds in the MDVs cause dramatic warming at onset and have significant effects on landscape forming processes; however, no detailed scientific investigation of foehn in the MDVs has been conducted. As a result, they are often misinterpreted as adiabatically warmed katabatic winds draining from the polar plateau. Herein observations from surface weather stations and numerical model output from the Antarctic Mesoscale Prediction System (AMPS) during foehn events in the MDVs are presented. Results show that foehn winds in the MDVs are caused by topographic modification of south-southwesterly airflow, which is channeled into the valleys from higher levels. Modeling of a winter foehn event identifies mountain wave activity similar to that associated with midlatitude foehn winds. These events are found to be caused by strong pressure gradients over the mountain ranges of the MDVs related to synoptic-scale cyclones positioned off the coast of Marie Byrd Land. Analysis of meteorological records for 2006 and 2007 finds an increase of 10% in the frequency of foehn events in 2007 compared to 2006, which corresponds to stronger pressure gradients in the Ross Sea region. It is postulated that the intra- and interannual frequency and intensity of foehn events in the MDVs may therefore vary in response to the position and frequency of cyclones in the Ross Sea region.


2021 ◽  
Author(s):  
◽  
Cassandra Anh Trinh-Le

<p>The hyper-arid, cryotic, wind-dominated conditions in the high-elevation McMurdo Dry Valleys of Antarctica are among Earth’s most extreme environments and represent the closest terrestrial analog to the surface of Mars. These unique conditions result in complex surface processes that occur in the overall absence of liquid water. However, since water is typically believed to be required for these processes to occur, the mechanisms responsible for how these processes can persist in this environment are poorly understood. Previous studies that focused on individual processes of sedimentation in the Dry Valleys leave questions regarding the role of water in dry cryotic sedimentation as well as the rates at which these processes occur. This thesis addresses these questions by combining Optically Stimulated Luminescence (OSL) dating, meteoric Beryllium-10 (10Be) measurements, soil geochemistry analysis, and petrographic microscopy analysis on ice-cemented permafrost cores taken from University Valley, one of the high-elevation Dry Valleys, where the availability and effects of liquid water are minimal. These analyses were used to explore four main sedimentation processes that occur in the Dry Valleys: chemical weathering, fine particle translocation, eolian transport, and physical weathering. Analyzed together, findings from these analyses comprehensively describe the complex processes involved in dry cryotic sedimentation and determine the roles of different phases of water in this environment.   Sediments in University Valley have accumulated at a rate of approximately 2.1 mm/ka for the last 200 ka, as dated by OSL, from erosion of the valley walls and deposition of windblown dust. Sediment accumulation is influenced by topography of the valley floor, depth of the ice table, aspect of the valley walls, wind direction, and mechanical breakdown of rocks due to solar heating. While persistent winds constantly remobilize fine particles and dust in the upper few cm of the dry ground, sediment grains that are sand-sized or larger do not undergo significant remobilization, and sediments in the ice-cemented ground are unaffected by remobilization and translocation processes. Rare clay bridges seen in thin section show that small, infrequent, transient surface wetting events have occurred over the last 200 ka. High anion concentrations associated with high surface meteoric 10Be measurements and clay bridges indicate that the source of these wetting events is the melting of wind-blown snow from coastal regions. Patterns in meteoric Be measurements show that these small transient wetting events are not sufficient to translocate fine particles through the soil profile, which suggests that the role of liquid water as a transporting agent is negligible in this environment. Chemical weathering in University Valley appears to be controlled by two main components: dolerite content of the sediments, and exposure to the atmosphere at the ground surface where condensation of water vapor onto grain surfaces readily leaches ions from dolerite grains under the oxidizing conditions of the Dry Valleys. In the absence of liquid water, chemical processes that occur in this environment rely on water vapor.   Together, these results indicate that surfaces in University Valley are remarkably young and sedimentologically active. Because University Valley represents one of the closest terrestrial analogs to the surface of Mars, findings from this thesis may be applicable to understanding the timescales and the processes that control anhydrous sedimentation on the surface of Mars.</p>


2004 ◽  
Vol 39 ◽  
pp. 139-145 ◽  
Author(s):  
Nancy A. N. Bertler ◽  
Paul A. Mayewski ◽  
Peter J. Barrett ◽  
Sharon B. Sneed ◽  
Michael J. Handley ◽  
...  

AbstractMcMurdo Dry Valleys (MDV; Ross Sea region, Antarctica) precipitation exhibits extreme seasonality in ion concentration, 3–5 orders of magnitude between summer and winter precipitation. To identify aerosol sources and investigate causes for the observed amplitude in concentration variability, four snow pits were sampled along a coast–Polar Plateau transect across the MDV. The elevation of the sites ranges from 50 to 2400 m and the distance from the coast from 8 to 93 km. Average chemistry gradients along the transect indicate that most species have either a predominant marine or terrestrial source in the MDV. Empirical orthogonal function analysis on the snow-chemistry time series shows that at least 57% of aerosol deposition occurs concurrently. A conceptual climate model, based on meteorological observations, is used to explain the strong seasonality in the MDV. Our results suggest that radiative forcing of the ice-free valleys creates a surface low-pressure cell during summer which promotes air-mass flow from the Ross Sea. The associated precipitating air mass is relatively warm, humid and contains a high concentration of aerosols. During winter, the MDV are dominated by air masses draining off the East Antarctic ice sheet, that are characterized by cold, dry and low concentrations of aerosols. The strong differences between these two air-mass sources create in the MDV a polar version of the monsoonal flow, with humid, warm summers and dry, cold winters.


2016 ◽  
Author(s):  
Devin Castendyk ◽  
◽  
Maciej K. Obryk ◽  
Sasha Z. Leidman ◽  
Michael Gooseff ◽  
...  

2016 ◽  
Author(s):  
Melisa A. Diaz ◽  
◽  
Susan A. Welch ◽  
Kathleen A. Welch ◽  
Alia L. Khan ◽  
...  

2016 ◽  
Author(s):  
Kate M. Swanger ◽  
◽  
Joerg M. Schaefer ◽  
Gisela Winckler

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