Hydrogen emission from moving solar prominences

Details Hydrogen emission from moving solar prominences Hydrogen emission from moving solar prominences

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..110..171h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 110, no. 1, 1987, p. 171-189.

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33

Balmer Series, Doppler Effect, Emission, Hydrogen, Solar Corona, Solar Prominences, Computational Astrophysics, Magnetohydrodynamics, Solar Magnetic Field, Velocity Distribution

Scientific paper

Brightness variations of the lines arising from a five-level hydrogen
model atom, depending upon prominence velocities, have been investigated
using a combination of two non-LTE techniques. The importance of the
Doppler brightening and/or Doppler dimming effects is demonstrated for
the lines of the Lyman and Balmer series.

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