Microturbulence near the edge of a solar plage

Details Microturbulence near the edge of a solar plage Microturbulence near the edge of a solar plage

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....89l...8s&link_type=abstract

Astronomy and Astrophysics, vol. 89, no. 1-2, Sept. 1980, p. L8, L9. Centre National d'Etudes Spatiales Centre National de la R

Physics

6

Atmospheric Turbulence, Faculae, K Lines, Solar Atmosphere, Solar Physics, Solar Activity Effects, Turbulence Effects

Scientific paper

Observations of the Ca II K line at the edge of a solar plage show
enhanced separation of the K2 peaks with respect to the measured value
inside the plage and in the quiet sun. This effect may be interpreted as
a variation of microturbulent motions at the height of formation of K2.

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