On the origin of subsecond pulses at 17 GHz

Details On the origin of subsecond pulses at 17 GHz On the origin of subsecond pulses at 17 GHz

Aug 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000soph..195..401a&link_type=abstract

Solar Physics, v. 195, Issue 2, p. 401-420 (2000).

Physics

11

Scientific paper

We have analyzed three flare events with subsecond structures in hard X-rays (CGRO/ BATSE) and 17 GHz data (Nobeyama radioheliograph). It was shown that microwave subsecond brightenings (SSB) were generated by directly precipitating electrons with energy of 100-200 keV from tiny regions close to footpoints. In two events, when high correlation between microwaves and X-rays was observed, the SSB can be interpreted in terms of gyrosynchrotron emission. Plasma emission seems to be a more credible explanation of the spontaneous pulses in the event when poor correlation with X-rays was observed.

Affiliated with

Also associated with

No associations

Rating

On the origin of subsecond pulses at 17 GHz does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On the origin of subsecond pulses at 17 GHz, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the origin of subsecond pulses at 17 GHz will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-893177