Theoretical NE V emission line ratios compared to solar observations

Details Theoretical NE V emission line ratios compared to solar observations Theoretical NE V emission line ratios compared to solar observations

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..105...47k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 105, May 1986, p. 47-50. SERC-supported research.

Physics

9

Emission Spectra, Line Spectra, Neon, Solar Spectra, Electron Orbitals, Solar Flares, Solar Prominences

Scientific paper

Using Ne V level population and A-values (Aggarwal, 1986), the I(DO-1De)/I(3DO 2-Pe 1) and I(1DO-1De)/I3DO 3-3Pe 2) theoretical line ratios are derived and compared with 171-630 A data for a solar flare and erupting prominence obtained with the Skylab NRL XUV spectrograph. The ratios are found to be in their high-density limits for electron densities typical of solar plasmas, and though they may not be used as density diagnostics for electron densities typical of solar transition region conditions, they are temperature dependent and can be employed in determining Te values for Ne V line emitting regions. The two ratios are consistent and found to be in good agreement with the predicted temperature of maximum Ne V abundance in ionization equilibrium (Arnaud and Rothenflug, 1985).

Affiliated with

Also associated with

No associations

Rating

Theoretical NE V emission line ratios compared to solar observations 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 Theoretical NE V emission line ratios compared to solar observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical NE V emission line ratios compared to solar observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1776407