Abstract
There are two kinds of bright threads in spectrograms of the Ca II H 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.
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© 1990 International Astronomical Union
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Suemoto, Z., Hiei, E. (1990). Bright Features In The Intergranular Region. In: Stenflo, J.O. (eds) Solar Photosphere: Structure, Convection, and Magnetic Fields. International Astronomical Union, vol 138. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1061-4_10
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DOI: https://doi.org/10.1007/978-94-009-1061-4_10
Publisher Name: Springer, Dordrecht
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