Intensity of lines from low-lying levels in C II, N III, O IV, NE VI, MG VIII, SI X, and SI II

Details Intensity of lines from low-lying levels in C II, N III, O IV, NE VI, MG VIII, SI X, and SI II Intensity of lines from low-lying levels in C II, N III, O IV, NE VI, MG VIII, SI X, and SI II

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...75..133c&link_type=abstract

Solar Physics, vol. 75, Jan. 1982, p. 133-137.

Physics

1

Chromosphere, Line Spectra, Solar Corona, Solar Spectra, Atomic Energy Levels, Collision Parameters, Ground State

Scientific paper

The populations of the excited state 2P 0 3/2 relative to the ground state 2P 0 1/2 are obtained, in a study of line intensities of the transition between those two states in C II, N III, O IV, Ne VI, Mg VIII, Si X, and Si II in the chromosphere-corona transition region, by considering all the radiative and collisional transition processes. The collisional transitions to the higher states which cascade to the upper level are included among these processes. It is found that the intensity, which may be expressed as a function of temperature alone, increases in the transition region with the charge on the ion for a sequence.

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