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NASA NTRS ยท 19900026034

Chromospheric heating

Abstract

The solar chromosphere is identified with the atmosphere inside magnetic flux tubes. Between the temperature minimum and the 7000 K level, the chromosphere in the bright points of the quiet sun is heated by large-amplitude, long-period, compressive waves with periods mainly between 2 and 4 minutes. These waves do not observe the cutoff condition according to which acoustic waves with periods longer than 3 minutes do not propagate vertically in the upper solar photosphere. It is concluded that the long-period waves probably supply all the energy required for the heating of the bright points in the quiet solar chromosphere.

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BibTeXRIS

Kalkofen, Wolfgang. 1989-11-01. Chromospheric heating. https://ntrs.nasa.gov/citations/19900026034

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