Common characteristics of the active regions of strong proton flares.

Details Common characteristics of the active regions of strong proton flares. Common characteristics of the active regions of strong proton flares.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ppmto..15..247z&link_type=abstract

Publ. Purple Mt. Obs., Vol. 15, No. 4, p. 247 - 252

Mathematics

Logic

Solar Active Regions: Solar Protons, Solar Active Regions: Solar Flares, Solar Protons: Solar Flares

Scientific paper

Common characteristics of nine active regions of strong proton flares in the 22th solar activity cycle have been studied. The results indicate that δ type sunspots with a single granular structure, that is many umbras with opposite magnetic polarities locked tightly in a single penumbra are typical morphological characteristics of the active regions of strong proton flares. Another important characteristics of the active regions of proton flares is the rotation of the sunspot groups.

Affiliated with

Also associated with

No associations

Rating

Common characteristics of the active regions of strong proton flares. 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 Common characteristics of the active regions of strong proton flares., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Common characteristics of the active regions of strong proton flares. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1172568