Theoretical population of the lower Zeeman levels relative to the 5303 line of Fe XIV

Details Theoretical population of the lower Zeeman levels relative to the 5303 line of Fe XIV Theoretical population of the lower Zeeman levels relative to the 5303 line of Fe XIV

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...41..373r&link_type=abstract

Solar Physics, vol. 41, Apr. 1975, p. 373-379. In French.

Physics

Atomic Spectra, Line Spectra, Population Theory, Solar Corona, Transition Probabilities, Zeeman Effect, Atomic Energy Levels, Atomic Excitations, Fine Structure, Iron, Particle Collisions, Polarized Radiation, Proton Impact, Solar Magnetic Field, Solar Wind

Scientific paper

The present paper presents in compact tabular form the relative population of the first six levels of the hyperfine structure of Fe XIV. These populations are calculated from the best atomic data presently available, in such a way as to establish a firm basis for the theoretical and observational interpretation of coronal polarization measurements.

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