Evolution of the X-ray emitting corona preceding and after major solar events

Details Evolution of the X-ray emitting corona preceding and after major solar events Evolution of the X-ray emitting corona preceding and after major solar events

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977cosp.meetr....w&link_type=abstract

COSPAR, Plenary Meeting, 20th, Tel Aviv, Israel, June 7-18, 1977, Paper. 12 p. Research supported by the Lockheed Independent R

Computer Science

Satellite Observation, Solar Corona, Solar Flares, Solar X-Rays, Electron Flux Density, Heliometers, Light Curve, Oso-8, Satellite-Borne Instruments

Scientific paper

Soft X-ray emission from the sun during STIP Interval II, observed with the Lockheed Mapping X-ray Heliometer on the NASA OSO-8 satellite, is presented. In examining the emission versus time for extended intervals around the times of the Class 1B flare on March 28, 1976, and the Class 1B flare on April 30, 1976, we find significantly more low level flare activity prior to the major flares than after. Twelve modest X-ray bursts are investigated and no compelling case of a preflare brightening phase is observed. Preliminary correlations with the time history of emitted solar particles are discussed.

Affiliated with

Also associated with

No associations

Rating

Evolution of the X-ray emitting corona preceding and after major solar events 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 Evolution of the X-ray emitting corona preceding and after major solar events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of the X-ray emitting corona preceding and after major solar events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1595429