Directivity of low frequency solar type 3 radio bursts

Details Directivity of low frequency solar type 3 radio bursts Directivity of low frequency solar type 3 radio bursts

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7611986f&link_type=abstract

Unknown

Physics

Directivity, Low Frequencies, Solar Activity, Solar Radio Bursts, Type 3 Bursts, Interplanetary Magnetic Fields, Satellite Observation, Solar Corona, Solar Physics, Solar Wind

Scientific paper

The occurrence rate of type 3 solar bursts in the frequency range 4.9 MHz to 30 kHz was analyzed as a function of burst intensity and burst arrival direction. Results show that: (1) the occurrence rate of bursts falls off with increasing flux and (2) the distribution of burst arrival directions at each frequency shows a significantly larger number of bursts observed west of the earth-sun line than east of it. This western excess in occurrence rate appears to be correlated with the direction of the average interplanetary magnetic field, and is interpreted as beaming of the observed burst radiation along the magnetic field direction.

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