Solar flares - The impulsive phase

Details Solar flares - The impulsive phase Solar flares - The impulsive phase

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121...75d&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Astronomy and Astrophysics

Astronomy

61

Energy Transfer, Solar Flares, Stellar Models, Energy Dissipation, Gamma Ray Astronomy, Radiation Distribution, Solar X-Rays, Ultraviolet Astronomy

Scientific paper

Only during the previous solar cycle have systematic observations begun to be made with the sensitivity and time resolution, and the continuous coverage required to catch the impulsive phase and measure the rapid variations present in many wavelength ranges. Observations in X-rays, gamma-rays, UV, H-alpha, and radio wavelengths all reveal rapid variations during the impulsive phase and have contributed to our understanding of the different phenomena involved. Results have been obtained from several spacecraft, from rocket and balloon flights, and from groung-based observations. These are reviewed in the context of a simple single loop flare model with a view to showing what results are consistent with this model and what the major problems are in understanding of the impulsive phase.

Affiliated with

Also associated with

No associations

Rating

Solar flares - The impulsive phase 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 Solar flares - The impulsive phase, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar flares - The impulsive phase will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1529356