On a strange recurring type I burst pattern

Details On a strange recurring type I burst pattern On a strange recurring type I burst pattern

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..107..123a&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 107, no. 1, 1987, p. 123-133.

Physics

1

Coronal Loops, Noise Storms, Solar Flux, Solar Radio Bursts, H Alpha Line, Magnetic Field Configurations, Solar Flares, Solar Magnetic Field, Solar X-Rays

Scientific paper

Two remarkable intensity-time patterns in the 113 and 64 MHz single-frequency radio flux records during a type I noise storm and/or a IV burst on July 31, 1983 are studied. A comparison of the patterns at both frequencies reveals a high degree of resemblance and an inherent common structure although the 64 MHz pattern was seen 40 min later than the 113 MHz pattern. An interpretation is given assuming a slowly uprising and thereby expanding clumpy plasma-magnetic field configuration which is (via accompanying coronal loops) illuminated two times by energetic electrons coming from the soft X-ray flare precursor source region of the H-alpha flares F1 and F2.

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