Analysis of X-ray line spectra from a transient plasma under solar flare conditions. I - General outline

Details Analysis of X-ray line spectra from a transient plasma under solar flare conditions. I - General outline Analysis of X-ray line spectra from a transient plasma under solar flare conditions. I - General outline

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....87..261m&link_type=abstract

Astronomy and Astrophysics, vol. 87, no. 3, July 1980, p. 261-268.

Astronomy and Astrophysics

Astrophysics

23

Line Spectra, Plasma Spectra, Solar Flares, Solar Spectra, Solar Wind, X Ray Spectra, Calcium, Iron, Plasma Equilibrium, Spectrum Analysis, Temperature Dependence, Time Dependence, Time Functions

Scientific paper

Complex iron and calcium spectra were computed as a function of time in the wavelength region (1.7 to 3.2 A) observable by the bent crystal spectrometer of the X-ray polychromator in the NASA Solar Maximum Mission. The computations were done on the basis of simple models with temperature-time courses considered as representative of the impulsive and gradual phases of solar flares. Results illustrate changes in the spectra with time and temperature.

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