The Use of High Frequency Solar Radar to Detect Coronal Mass Ejections

Details The Use of High Frequency Solar Radar to Detect Coronal Mass Ejections The Use of High Frequency Solar Radar to Detect Coronal Mass Ejections

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998stin...9994172p&link_type=abstract

Technical Report, AD-A353482; EOARD-SPC-97-4078 Radiophysical Research Inst.

Physics

High Frequencies, Solar Corona, Stellar Mass, Stellar Mass Ejection, Radar Tracking, Solar Activity

Scientific paper

This report results from a contract tasking Radiophysical Research Institute (NTRFI) as follows: The contractor will investigate techniques of high frequency solar radars and receiving antennas to detect mass motions in the solar corona such as solar mass ejections. Testing will be accomplished and solar data taken using the Sura Radar Facility and the UTR-2 Receiving Antenna as described in the proposal.

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