Density dependence of the line emission of boron-like coronal ions

Details Density dependence of the line emission of boron-like coronal ions Density dependence of the line emission of boron-like coronal ions

Dec 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..38..369e&link_type=abstract

(International Astronomical Union, Colloquium on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas, Cambridge, M

Astronomy and Astrophysics

Astrophysics

14

Electron Density (Concentration), Emission Spectra, Ion Emission, Solar Corona, Boron, Electron Energy, Infrared Spectra, Solar Electrons, Solar X-Rays, Steady State, Ultraviolet Spectra

Scientific paper

Assuming steady-state conditions, the occupation of 20 levels of the ion Si X is calculated as a function of the electron density and temperature taking into account collisional processes and spontaneous radiative ones. Between the two levels of the ground state, the photo-absorption of the corresponding infrared radiation has been considered. The emission of the most important UV, X-ray, and IR lines is determined as a function of the electron density and temperature. Intensity ratios are plotted against electron density. Line emission as a function of the height of the radiating layers is studied for UV and X-ray lines. The resulting fluxes at 1 AU are compared with observations.

Affiliated with

Also associated with

No associations

Rating

Density dependence of the line emission of boron-like coronal ions 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 Density dependence of the line emission of boron-like coronal ions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Density dependence of the line emission of boron-like coronal ions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1576659