Physics
Scientific paper
Jun 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998kfnt...14..234k&link_type=abstract
Kinematika Fiz. Nebesn. Tel, Tom 14, No. 3, p. 234 - 244
Physics
Solar Flares: Solar Plages, Solar Flares: Solar Photosphere, Solar Flares: Fraunhofer Lines
Scientific paper
The authors analyse four Fraunhofer lines in the spectra of the solar flare (the main phase), the plage, and the surrrounding photosphere. The changes of the depth, width, equivalent width of the line profiles, the line asymmetry and shifts depend on the line formation height. The decrease in the line central depths and equivalent widths of the flare and plage and their increase in the surrounding photosphere were observed. Differences of line shifts measured in flare and plage spectra were found. Observed variations in the photospheric layers are probably caused by the passage of the chromospheric condensation and by the waves formed during the flare.
Kondrashova N. N.
Pasechnik M. N.
No associations
LandOfFree
The photospheric layers of the flare and the plage. II. Profiles, asymmetry, and shifts of the Fraunhofer lines in the near-by regions spectra. 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 photospheric layers of the flare and the plage. II. Profiles, asymmetry, and shifts of the Fraunhofer lines in the near-by regions spectra., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The photospheric layers of the flare and the plage. II. Profiles, asymmetry, and shifts of the Fraunhofer lines in the near-by regions spectra. will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1334465