The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XII

Details The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XII The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XII

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...227.1037c&link_type=abstract

Astrophysical Journal, Part 1, vol. 227, Feb. 1, 1979, p. 1037-1046.

Astronomy and Astrophysics

Astronomy

89

Forbidden Bands, Solar Corona, Solar Spectra, Spectral Line Width, Ultraviolet Astronomy, Emission Spectra, Far Ultraviolet Radiation, Iron, Magnetohydrodynamic Waves, Propagation Modes, Silicon

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1979ApJ...227.1037C

Affiliated with

Also associated with

No associations

Rating

The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XII 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 dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XII, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XII will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828994