Background

The St. Olaf College contribution to the US-ITASE 2 program is a deep-penetrating 3 MHz radio echo-sounding system that can measure the bedrock surface beneath the ice as well as internal layers that have unique electrical properties.  Total ice thickness data is useful to researchers who develop ice-flow models of the ice sheet.  The immense size of the ice sheet makes it difficult to obtain high-accuracy thickness measurements over the entire continent.  The long distance traverses of the US-ITASE program make it an ideal platform for ground-based radar measurements.

Internal ice reflections are usually related to deposition of volcanic debris (acids or ash) or dust layers.  These layers give researchers a window into the accumulation and flow history of the ice sheet.  Changes in the layer thickness along the traverse routes may be attributed to changes in snow accumulation due to climate or geographic changes (crossing a drainage divide, for example).  Changes in the ice flow velocity due to bumps in the bedrock or changes in the bedrock character cause the ice to thicken or thin as the ice decelerates or accelerates.

We plan to resurvey a number of radar profiles recorded at Taylor Dome by David Morse and Howard Conway from the Univ. of Washington prior to the Taylor Dome Ice Core project in the early 1990's. These profiles will help us establish a baseline for the reflectivity of bedrock frozen to the ice sheet and also provide dates for internal ice layers. Once the traverse departs Taylor Dome we will record radar profiles along the entire traverse route to establish dating control of the internal stratigraphy that can be traced back to the Taylor Dome core. We plan to collect radar profiles on a number of side-traverses that will parallel ice flow in order to examine the influence of basal conditions on flow dynamics. In addition we hope to gain access to a number of the ridges separating the large outlet glaciers that drain the East Antarctic Ice Sheet through the Transantarctic Mountains to examine the stability of ice flow into the glaciers. Finally we will visit a number of interesting glaciological features along the route including Titan Dome, large zones of wind erosion, and perhaps the edges of the Mega-dunes region. Our 3 MHz radar system has been upgraded to collect data closer to the ice surface so we hope to correlate our internal ice stratigraphy with that collected by Steve Arcone's 400 MHz shallow radar system. Upon reaching the South Pole in Year 2 of this project we will connect our radar stratigraphy to the data collected in West Antarctica during the first phase of US-ITASE (1999-2003) that also finished at South Pole.

Map of the proposed traverse corridor for US-ITASE 2 starting at Taylor Dome and ending at South Pole. Click the map for a full-size image.

Results, Publications & Data

Results of the project will be posted here soon after the first field season. As we publish our findings we will post relevant data sets at the National Snow & Ice Data Center.

US-ITASE 2006:

The traverse route started at Taylor Dome near the Transantarctic Mts. just west of McMurdo Station. The route headed inland and then turned south 130 km from Taylor Dome. We continued south into the Byrd Glacier drainage, collecting ice cores at four sites as well as over 500 km of deep (3 MHz) and shallow (400 MHz) radar data. Logistical problems limited our travel distance this year, but we still made good progress and expect to make it to South Pole in 2007.

US-ITASE 2007:

Instrumentation & Methods

We operate a 3 MHz radio echo-sounding system to transmit and receive radio waves through as much as 3.5 km of ice.  This signal frequency translates to a wavelength of about 56 m in ice.  The transmitter (made by the Kentech) emits pulses at frequency of up to 2 kHz.  The pulses are emitted by our transmitter antenna, a 40 m dipole dragged along the snow surface.  135 m in front of the transmitter is an identical dipole antenna that receives the signal.  The signal is amplified and passed on to an oscilloscope board mounted directly on a field-ready PC computer.  The scope board identifies the incoming signal, digitizes it, and sends it to the computer to be stored on the hard drive.  The scope board is extremely fast, sampling the signal at up to 200 million samples/second.  Each sample of the signal is digitized to a 14-bit value and stored on the computer along with the recording parameters and a precise time-stamp.

We use the scope board's speed to stack the incoming signal to remove much of the environmental radio noise that hides our reflected signal.  We stack the data in the field by averaging about a thousand of the transmitter pulses and their resultant echoes from the bedrock and internal layers.  The traverse train travels at about 12 km/hr so we generally stack 1200-1500 pulses in order to record a trace every few meters.  Stacking and the fast scope board allow us record a dense profile of traces while eliminating much of the noise that would make the data difficult to process and interpret.

More about basic radio echo-sounding techniques

Field Logistics

Our radar system operates primarily during the traverses between ice coring sites (map of the proposed route).  The system and operator are towed as the very last sleds in the traverse train to eliminate radio noise from other instrumentation or reflections from the metal sleds and equipment.  The receiver and operator are housed in a small shelter built on a wooden Komatik sled.  The shelter protects the computer and operator from wind, cold, and snow.  Power for the receiver can be derived from a solar-powered battery system, or a small gasoline-powered generator mounted on the back of the sled.  Batteries to power the transmitter are charged by the solar panels or the generator.  The shelter is also equipped with a GPS receiver to geolocate the radar data.  A survival bag is strapped to the front of the shelter in case of emergency.

The transmitter is towed 135 m or more behind the receiver sled.  The transmitter and its battery sit in a small sled and are protected from the elements by the sled's nylon cover.  The antennas for the transmitter and receiver are housed in strong hydraulic hoses and tied to the tow ropes to keep the antennas as straight and parallel as possible.

Picture of the receiver sled & transmitter sled used in US-ITASE 1
Picture of the interior of the receiver shelter used in US-ITASE


©2008, CEGSIC, St. Olaf College
Last Updated: January 25, 2008