Heights of formation of non-magnetic solar lines suitable for velocity studies

Details Heights of formation of non-magnetic solar lines suitable for velocity studies Heights of formation of non-magnetic solar lines suitable for velocity studies

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...43...33a&link_type=abstract

Solar Physics, vol. 43, July 1975, p. 33-37.

Physics

25

Line Spectra, Solar Magnetic Field, Solar Spectra, Velocity Distribution, Atmospheric Turbulence, Photosphere, Solar Activity, Thermodynamic Equilibrium, Zeeman Effect

Scientific paper

Heights of formation of lines that do not exhibit Zeeman splitting are calculated using LTE, partial non-LTE, and full non-LTE approaches. Nonmagnetic (g equals 0) lines are valuable for velocity investigations in quiet-sun magnetic-field regions, and a knowledge of their formation heights is useful for obtaining three-dimensional velocity profiles in these regions.

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