Brightness temperatures and polarizations of solar active regions at 3.8 cm, theory and observations

Details Brightness temperatures and polarizations of solar active regions at 3.8 cm, theory and observations Brightness temperatures and polarizations of solar active regions at 3.8 cm, theory and observations

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975bosu.rept.....p&link_type=abstract

Final Report, 1 Sep. 1972 - 30 Jun. 1975 Boston Univ., MA. Dept. of Astronomy.

Astronomy and Astrophysics

Astronomy

Brightness Temperature, Polarized Electromagnetic Radiation, Solar Activity, Solar Radio Emission, Earth Ionosphere, Earth Magnetosphere, Extraterrestrial Radiation, Pattern Recognition, Polarization Characteristics, Solar Flares

Scientific paper

Extensive observations (230 hours in 1973 and 1974) of right and left circularly polarized emission from solar active regions were carried out at 3.8 cm with the 120 ft Haystack antenna, which at this frequency has a resolution of about 4.4 arc minutes. The purpose of these observations was to study the changes in brightness temperature and polarization before flare activity in the hope of recognizing characteristic patterns which could be used as warning signals in the forecasting of major solar flare events.

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