Observations of small solar flares with BATSE

Details Observations of small solar flares with BATSE Observations of small solar flares with BATSE

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aipc..294..183b&link_type=abstract

High energy solar phenomena-A new ear of spacecraft measurements. AIP Conference Proceedings, Volume 294, pp. 183-186 (1994).

Other

4

Scientific paper

The Burst and Transient Source Experiment on board the Compton Gamma Ray Observatory is being used to observe solar flares. The Large Area Detectors are sensitive to small solar flares. We are searching the BATSE data for solar flares with an automated algorithm that allows for independent confirmation of the event origin. With this search method, we have detected solar flares almost an order of magnitude smaller than those found in a visual search of the BASTE data. We present results that are consistent with the differential distribution of peak flare rates observed by other researchers. These results show that the rate of occurrence of the smallest flares observed by BATSE can be predicted from the rate of occurrence of larger flares.

Affiliated with

Also associated with

No associations

Rating

Observations of small solar flares with BATSE 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 Observations of small solar flares with BATSE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations of small solar flares with BATSE will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1325198