Other
Scientific paper
Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...261..684a&link_type=abstract
Astrophysical Journal, Part 1, vol. 261, Oct. 15, 1982, p. 684-699.
Other
33
Chromosphere, Coronal Loops, Solar Corona, Solar Magnetic Field, Sunspots, Atmospheric Circulation, Brightness Distribution, Circulation Distribution, Doppler Effect, Flow Velocity, Magnetic Field Configurations, Magnetohydrodynamic Flow, Solar Atmosphere, Solar Spectra, Steady Flow
Scientific paper
From a study of Dopplergrams made with two narrow slits in the opposite wings of the C IV line, N λ1548, we find widespread evidence for steady flow patterns associated with large sunspots and, on a larger scale, with active region magnetic field patterns. The characteristic sunspot flow is in the reverse Evershed sense with a substantial vertical component. Active region flows indicate oppositely directed velocities with mainly horizontal components on either side of magnetic neutral lines. Some neutral lines show flow toward the neutral line, whereas others show flow away from the neutral line.
Athay Grant R.
Gurman Joe B.
Henze William
Shine Richard A.
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