The sun's chromospheric velocity field as inferred from the CA II K line

Details The sun's chromospheric velocity field as inferred from the CA II K line The sun's chromospheric velocity field as inferred from the CA II K line

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....51...95d&link_type=abstract

Astronomy and Astrophysics, vol. 51, no. 1, Aug. 1976, p. 95-99.

Astronomy and Astrophysics

Astrophysics

16

Abundance, Calcium, Chromosphere, K Lines, Shock Wave Propagation, Solar Atmosphere, Velocity Distribution, Acoustic Propagation, Atmospheric Models, Coherent Scattering, Hertzsprung-Russell Diagram, High Resolution, Propagation Velocity, Spatial Distribution, Standing Waves, Traveling Waves

Scientific paper

Theory and observation of the solar Ca II K line under high spatial resolution are briefly reviewed. It is shown that contrary to popular belief, present theory is not capable of explaining the observed features of the K line. An attempt is made to develop a schematic model of the temporal behavior of the spatially resolved K line, based on Leibacher's (1971) investigation of waves in the solar atmosphere

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