Density dependence of solar emission lines of boron-like ions

Details Density dependence of solar emission lines of boron-like ions Density dependence of solar emission lines of boron-like ions

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980soph...68..111d&link_type=abstract

(Astronomical Society of India, Meeting, 5th, Naini Tal, India, Nov. 5-9, 1979.) Solar Physics, vol. 68, Nov. 1980, p. 111-123.

Physics

18

Boron, Electron Density (Concentration), Line Spectra, Metal Ions, Solar Atmosphere, Solar Spectra, Abundance, Extreme Ultraviolet Radiation, Magnesium, Radiative Transfer, Silicon, Solar Physics, Spectroheliographs, Temperature Effects, Ultraviolet Spectra

Scientific paper

Steady state level densities of 20 levels of the boron-like ions Mg VII and Si X have been computed as a function of electron density and temperature. Collisional and spontaneous radiative processes have been accounted for. Photoexcitation between the two levels of the ground term has also been considered. Using the computed level density line intensities have been obtained as a function of electron density and temperature. In case of Mg VII, the line intensity ratio I(430.47)/I(436.62) is found to be electron density sensitive. Likewise other pairs of lines, namely, I(75.03)/I(74.86), I(315.02)/I(430.47), and I(315.02)/I(335.23) are also found to be density sensitive. Similar density-sensitive line intensity ratios have been found for Si X. Absolute line fluxes from these ions at earth distance have been computed and are found to be comparable with values obtained using various satellite and rocket measurements.

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