Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26as...40..323m&link_type=abstract
Astronomy and Astrophysics Supplement Series, vol. 40, June 1980, p. 323-346.
Astronomy and Astrophysics
Astrophysics
32
Line Spectra, Nonuniform Plasmas, Plasma Spectra, Solar Flares, Spectrum Analysis, X Ray Spectroscopy, Continuous Radiation, Electron Density (Concentration), Electron Energy, High Temperature Plasmas, Ion Recombination, Ionization Coefficients, Plasma Diagnostics, Radiative Recombination, Recombination Coefficient, Solar Spectra, Tables (Data)
Scientific paper
The rate coefficients for ionization, recombination, excitation, etc.,
needed for the calculations of high-resolution X-ray line spectra in
the wavelength range 1.7-3.2 Å from highly ionized iron and
calcium atoms have been presented.
Mewe Rolf
Schrijver J.
Sylwester Janusz
No associations
LandOfFree
Analysis of X-ray line spectra from a transient plasma under solar flare conditions. II - Rate coefficients. III - Diagnostics for measuring electron temperature and density 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 Analysis of X-ray line spectra from a transient plasma under solar flare conditions. II - Rate coefficients. III - Diagnostics for measuring electron temperature and density, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Analysis of X-ray line spectra from a transient plasma under solar flare conditions. II - Rate coefficients. III - Diagnostics for measuring electron temperature and density will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1214413