The variation of line asymmetry during the solar flare of October 7, 1979

Details The variation of line asymmetry during the solar flare of October 7, 1979 The variation of line asymmetry during the solar flare of October 7, 1979

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kfnt....4...23k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 4, July-Aug. 1988, p. 23-28. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Fraunhofer Lines, Solar Flares, Asymmetry, Flow Velocity, Photosphere, Vertical Motion

Scientific paper

The fine structure of Fraunhofer lines observed during the flare of October 7, 1979 is studied. The line asymmetry is shown to be dependent on the formation depth of the lines and on the flare phase. The observed variations may be explained by an increase in the velocity of the ascent of matter in the photospheric and chromospheric layers in the initial phase of the flare and by its subsequent descent.

Affiliated with

Also associated with

No associations

Rating

The variation of line asymmetry during the solar flare of October 7, 1979 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 The variation of line asymmetry during the solar flare of October 7, 1979, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The variation of line asymmetry during the solar flare of October 7, 1979 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1695065