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Wave Heating in Magnetic Flux Tubes

Published online by Cambridge University Press:  08 February 2017

Wolfgang Kalkofen
Wolfgang Kalkofen*
Affiliation:
Harvard-Smithsonian Center for Astrophysics 60 Garden Street, Cambridge, Massachussetts 02138

Abstract

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The solar chromosphere is identified with the atmosphere inside magnetic flux tubes. In the quiet sun, the layers of the low and middle chromosphere are heated by compressive waves with periods mainly between 2 min and 4 min. These long-period waves probably supply all the energy required for the heating of the quiet solar chromosphere.

Type
III. Small-Scale Magnetic Fields
Information
Symposium - International Astronomical Union , Volume 138: Solar Photosphere: Structure, Convection and Magnetic Fields , 1990 , pp. 185 - 188
Copyright
Copyright © Kluwer 1990 

References

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