Observational Study of Macroscopic Inhomogeneities in the Solar Atmosphere. I. Velocity Displacements of Fraunhofer Lines as a Function of Line Strength and Position on Disk.

Details Observational Study of Macroscopic Inhomogeneities in the Solar Atmosphere. I. Velocity Displacements of Fraunhofer Lines as a Function of Line Strength and Position on Disk. Observational Study of Macroscopic Inhomogeneities in the Solar Atmosphere. I. Velocity Displacements of Fraunhofer Lines as a Function of Line Strength and Position on Disk.

May 1962

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1962apj...135..812e&link_type=abstract

Astrophysical Journal, vol. 135, p.812

Astronomy and Astrophysics

Astrophysics

45

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1962ApJ...135..812E

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