High-Order Hydrogen Balmer Profiles in Solar Flares. The Structure of the Emission Region

Details High-Order Hydrogen Balmer Profiles in Solar Flares. The Structure of the Emission Region High-Order Hydrogen Balmer Profiles in Solar Flares. The Structure of the Emission Region

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985baicz..36..378s&link_type=abstract

Bulletin of the Astronomical Institute of Czechoslovakia, vol. 36, p.378

Astronomy and Astrophysics

Astronomy

Scientific paper

The emission profiles of hydrogen lines H7, H8, H10 H11 and H12 in the solar flare of Aug. 18, 1958 are investigated. From the shape of the line profiles at various times of observations, one can draw conclusions about their generation under rotations of clots of matter about a general axis, the Doppler velocity of which grows with the distance from the axis and the density decreases.

Affiliated with

Also associated with

No associations

Rating

High-Order Hydrogen Balmer Profiles in Solar Flares. The Structure of the Emission Region 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 High-Order Hydrogen Balmer Profiles in Solar Flares. The Structure of the Emission Region, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-Order Hydrogen Balmer Profiles in Solar Flares. The Structure of the Emission Region will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-978094