Brightness fluctuations of solar ultraviolet line intensities during a shock-wave passage

Details Brightness fluctuations of solar ultraviolet line intensities during a shock-wave passage Brightness fluctuations of solar ultraviolet line intensities during a shock-wave passage

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979soph...61..389p&link_type=abstract

Solar Physics, vol. 61, Mar. 1979, p. 389-405.

Physics

5

Atmospheric Models, Shock Wave Propagation, Solar Atmosphere, Solar Spectra, Stellar Spectrophotometry, Ultraviolet Spectra, Abundance, Brightness, Ions, Line Spectra, Neon, Time Dependence

Scientific paper

A simplified method is developed to derive the modifications induced at successive times by the passage of a shock wave in a standard unperturbed transition-region solar atmosphere. Time-dependent 'shocked' models allow the evaluation of the effects of the vertically propagating shock wave on the intensity of UV lines. Out-of-equilibrium effects are taken into account to evaluate time-varying ion abundances. The behavior of the modified UV intensities is compared with the experimental results of Vernazza et al. (1975).

Affiliated with

Also associated with

No associations

Rating

Brightness fluctuations of solar ultraviolet line intensities during a shock-wave passage 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 Brightness fluctuations of solar ultraviolet line intensities during a shock-wave passage, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Brightness fluctuations of solar ultraviolet line intensities during a shock-wave passage will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-809625