Profile Fluctuations in the Wings of the λ5183.6 Mg b Line Due to Solar Photospheric Inhomogeneities

Details Profile Fluctuations in the Wings of the λ5183.6 Mg b Line Due to Solar Photospheric Inhomogeneities Profile Fluctuations in the Wings of the λ5183.6 Mg b Line Due to Solar Photospheric Inhomogeneities

Jan 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971baas....3....6e&link_type=gif

Bulletin of the American Astronomical Society, Vol. 3, p.6

Astronomy and Astrophysics

Astronomy

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