The characteristics of the solar microwave bursts of June 30, 1989.

Details The characteristics of the solar microwave bursts of June 30, 1989. The characteristics of the solar microwave bursts of June 30, 1989.

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ppmto..10..114y&link_type=abstract

Publ. Purple Mt. Obs., Vol. 10, No. 2, p. 114 - 121

Other

Scientific paper

The two-peak strucutre, spectral characteristics, and time-delay of the microwave burst event of June 30, 1989 are described and analysed. (1) There were time delays of the two peaks from the high frequencies to low frequencies (1 - 15 GHz). The high frequency peak time preceded the low frequency peak time for 84 s. It seems that the efficiency of particle acceleration at the two peaks is different each other. (2) This event accompanied the proton event. (3) The spectral indices of two peaks at 9400 MHz and 3750 MHz changing with time were consistent with the time profile of the burst 9375 MHz.

Affiliated with

Also associated with

No associations

Rating

The characteristics of the solar microwave bursts of June 30, 1989. 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 The characteristics of the solar microwave bursts of June 30, 1989., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The characteristics of the solar microwave bursts of June 30, 1989. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1277475