Characteristics of the Linear Polarization Observed in the 16 May 1991 Solar Flare

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

12

Polarization, Flare

Scientific paper

In a search for linear polarization effects, 37 profiles of the H α line emitted in the 16 May 1991 flare have been analyzed. Linear polarization is clearly present in the central part of line. On average, the degree of polarization is 7 %, but it reaches 20 % in regions with lower H ga emission. Generally the orientation of the plane of polarization coincides with the flare to disk center direction, except for sections where the H ga line has the characteristic form observed in moustaches. We believe that the linear polarization observed in the 16 May 1991 flare was caused by bombardment of the chromosphere by beams of accelerated particles, protons in the main part of the flare and electrons at locations where the H ga line has the characteristic moustache structure.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Characteristics of the Linear Polarization Observed in the 16 May 1991 Solar Flare 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 Characteristics of the Linear Polarization Observed in the 16 May 1991 Solar Flare, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characteristics of the Linear Polarization Observed in the 16 May 1991 Solar Flare will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1618065

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.