Atomic Physics Calculations Relevant to Solar Flare Spectra

Details Atomic Physics Calculations Relevant to Solar Flare Spectra Atomic Physics Calculations Relevant to Solar Flare Spectra

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991rspta.336..471m&link_type=abstract

Philosophical Transactions: Physical Sciences and Engineering, Volume 336, Issue 1643, pp. 471-484

Physics

3

Scientific paper

Solar flare spectra in the ultraviolet and X-ray wavelength regions are rich in emission lines from highly ionized ions, formed at temperatures around 107 K. These lines can be used as valuable diagnostics for probing the physical conditions in solar flares. Such analyses require accurate atomic data for excitation, ionization and recombination processes. In this paper, we present a review of work which has already been carried out, in particular for the Solar Maximum Mission observations, and we look to future requirements for Solar-A.

Affiliated with

Also associated with

No associations

Rating

Atomic Physics Calculations Relevant to Solar Flare 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 Atomic Physics Calculations Relevant to Solar Flare Spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atomic Physics Calculations Relevant to Solar Flare Spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-898341