Motions in solar magnetic tubes. I - The downflow

Details Motions in solar magnetic tubes. I - The downflow Motions in solar magnetic tubes. I - The downflow

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...57..255g&link_type=abstract

Solar Physics, vol. 57, Apr. 1978, p. 255-260.

Physics

28

Faculae, Flow Velocity, Gas Flow, Magnetic Signatures, Solar Magnetic Field, Line Spectra, Magnetic Measurement, Vertical Motion

Scientific paper

The line-center-magnetogram technique has been used to measure the average velocity in magnetic elements in plages and isolated magnetic elements (including dipoles) in Ca II 8542, Mg I 5183, Fe I 8688 and C I 9111. The velocities vary from 0.6 km/s downflow in the line of deepest origin to zero in the highest. The smooth curve obtained by combining these with the results of other investigators is in conformity with Giovanelli's (1977) theory of inflow in the neighborhood of the temperature minimum.

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