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The Amundsen–Scott South Pole Station is a United States scientific research station at the South Pole of the Earth. It is the southernmost point under the jurisdiction (not sovereignty) of the United States. The station is located on the high plateau of Antarctica at 9,301 feet (2,835 m) above sea level.
The South Pole Traverse, also called the South Pole Overland Traverse, [2] is an approximately 995-mile-long (1,601 km) flagged route over compacted snow and ice [3] in Antarctica that links McMurdo Station on the coast to the Amundsen–Scott South Pole Station, both operated by the National Science Foundation of the United States. [4]
The Amundsen–Scott South Pole Station recorded its warmest average July temperature since 2002 at 6.3 °C (11.3 °F) above average, with an average temperature of −47.6 °C (−53.7 °F) from 20 to 30 July, meeting the average February Antarctic temperature at the typical end of summer.
The IceCube Neutrino Observatory (or simply IceCube) is a neutrino observatory developed by the University of Wisconsin–Madison and constructed at the Amundsen–Scott South Pole Station in Antarctica. [1] The project is a recognized CERN experiment (RE10).
Locations of all known installed Antarctic automatic weather stations as of 2009 Current locations of all known installed Antarctic automatic weather stations. Data from the UW-Madison Antarctic AWS program has been used for many research studies including, but not limited to: boundary layer meteorology studies near the South Pole, Katabatic wind studies at Reeves Glacier and the Adelie Coast ...
The Ceremonial South Pole. 300 Club participants walk briskly from the Amundson-Scott station to this marker, circle it, and then return to the station wearing only boots. Participants in the Antarctic 300 Club wait for a winter day when the temperature drops to −100 °F (−73 °C). This can happen in April to September (see South Pole).
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The South Pole Telescope (SPT) is a 10-metre (390 in) diameter telescope located at the Amundsen–Scott South Pole Station, Antarctica.The telescope is designed for observations in the microwave, millimeter-wave, and submillimeter-wave regions of the electromagnetic spectrum, with the particular design goal of measuring the faint, diffuse emission from the cosmic microwave background (CMB). [5]