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Bright Features in the Intergranular Region

Published online by Cambridge University Press:  08 February 2017

Z. Suemoto  and
E. Hiei
Z. Suemoto
Affiliation:
National Astronomical Observatory Mitaka, Tokyo 181 Japan
E. Hiei
Affiliation:
National Astronomical Observatory Mitaka, Tokyo 181 Japan

Abstract

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There are two kinds of bright threads in spectrograms of the Ca II II and K lines: the ones in the outer line wing are due to enhancements of the continuum inside granules, while the others in the inner wing are due to bright features in the intergranular regions.

Type
II. Photospheric Fine Structure
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 97 - 100
Copyright
Copyright © Kluwer 1990 

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