Solar energetic particles and wide-band continuum storms from metric to hectometric frequencies

Details Solar energetic particles and wide-band continuum storms from metric to hectometric frequencies Solar energetic particles and wide-band continuum storms from metric to hectometric frequencies

Jan 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973p%26ss...21...17s&link_type=abstract

Planetary and Space Science, Volume 21, Issue 1, p. 17-22.

Computer Science

1

Scientific paper

In association with solar flares accompanying type IV radio bursts of U-shaped spectrum, solar cosmic rays (MeV) and energetic electrons (keV) were generated. After acceleration, they were first stored in or near the flare regions and then gradually emitted into outer space. It seems that the streams of keV electrons generated the continuum radio emissions from metric to hectometric frequencies while passing through the outer coronal regions. sNASA Associate with University of Maryland.

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