An interpretation of a HXR flare with exceedingly long delay

Details An interpretation of a HXR flare with exceedingly long delay An interpretation of a HXR flare with exceedingly long delay

Feb 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001acasn..42...47l&link_type=abstract

Acta Astronomical Sinica, vol.42, no.1, p. 47-53.

Astronomy and Astrophysics

Astronomy

1

Solar Flare, Hard X-Ray, Delay

Scientific paper

The HXR peak delay of 3B flare of March 6, 1989 (1354-1624UT) is about 130 seconds, while the rising time of the lowest energy channel of X-rays is only 150 seconds. The authors use the trap plus precipitation model to explain this unprecedented and peculiar event. It is found that it can be well interpreted if two successive sources are involved and coronal density is taken to be 109 cm-3.

Affiliated with

Also associated with

No associations

Rating

An interpretation of a HXR flare with exceedingly long delay 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 An interpretation of a HXR flare with exceedingly long delay, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An interpretation of a HXR flare with exceedingly long delay will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1711500