The Influence of Molecular Blends and Non-Thermal Line Broadening on the Profile of the Zeeman Triplet λ5250.22 in Sunspots

Details The Influence of Molecular Blends and Non-Thermal Line Broadening on the Profile of the Zeeman Triplet λ5250.22 in Sunspots The Influence of Molecular Blends and Non-Thermal Line Broadening on the Profile of the Zeeman Triplet λ5250.22 in Sunspots

Dec 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973soph...33..393m&link_type=abstract

Solar Physics, Volume 33, Issue 2, pp.393-401

Physics

1

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1973SoPh...33..393M

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