2003-2004 USAP Field Season

Aeronomy & Astrophysics

Dr. Vladimir Papitashvili
Program Manager

A-100-M

NSF/OPP 01-38126
Station: McMurdo Station
RPSC POC: Charles Kaminski
Research Site(s): McMurdo Station
Dates in Antarctica: Instruments operate year-round

The Operation of an ELF/VLF Radiometer at Arrival Heights, Antarctica
Dr. Antony C. Fraser-Smith
Stanford University
STAR Laboratory
acfs@alpha.stanford.edu
 
View from the ELF/VLF radio antenna on the "Second Crater" at Arrival Heights. Mt. Discovery provides a backdrop for the New Zealand communications satellite installation on top of the "First Crater." US (white) and New Zealand (green) huts are also vis
Research Objectives: Since it was discovered in the 1930s that natural phenomena emit the lowest form of electromagnetic energy (radio waves), the field of radio astronomy has joined the scientific effort to analyze both atmospheric and extraterrestrial signals. The extremely-low-frequency and very-low-frequency (ELF/VLF) record of data collected by this project at Arrival Heights-chosen because it is unusually free from manmade electromagnetic interference-now extends unbroken for almost 15 years.

The radiometers at McMurdo operate in both the ELF and VLF ranges, monitoring radio noise from natural sources such as thunderstorms. Characterizing the possible sources of radio interference is important for operational purposes. Since thunderstorms generate telltale radio signals, tracking variations in global noise reflects thunderstorm activity and thus can provide information on changes in global climate.

The Arrival Heights site is one of a network of eight such radiometers operated by Stanford University for the Office of Naval Research.