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...9994136k&link_type=abstract

Technical Report, AD-A353796; EOARD-SPC-97-4079 Dept. of Decametric Radio Astronomy

Astronomy and Astrophysics

Astronomy

Solar Observatories, Solar Corona, Solar Physics, Radio Astronomy, Solar Radiation, Stellar Mass Ejection, Radar Data, Radar Imagery, Radio Telescopes

Scientific paper

This report results from a contract tasking Institute of Radio Astronomy (RIAN) as follows: The contractor will investigate the usable frequencies and effective radiated powers required to penetrate the ionosphere, reach the sun and return at detectable levels; the best duty cycles and waveforms needed to coordinate Sura radar operations with the UTR-2 antenna and the ionospheric effect on transmitted radar waves. Radar tests planned for the Sura and UTR-2 facilities will be correlated with various solar monitoring observatories providing images of the solar corona and the solar disk. All work is to be performed as described in the proposal.

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