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.

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..107..123a&link_type=abstract

Solar Physics, Volume 107, Issue 1, pp.123-133

Physics

Solar Radio Bursts

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 type IV burst on 31 July, 1983 are studied. A comparison of the patterns at both frequencies reveals a high degree of resemblance and 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) two times illuminated by energetic electrons coming from the soft X-ray flare precursor source region of the H-alpha flares F1 and F2 (see Figure 1).

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