Coronal-hole cycle variations of basic heliosphere quantities and coronal hole atmosphere.

Details Coronal-hole cycle variations of basic heliosphere quantities and coronal hole atmosphere. Coronal-hole cycle variations of basic heliosphere quantities and coronal hole atmosphere.

Jan 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11...46z&link_type=abstract

Chin. J. Space Sci., Vol. 11, No. 1, p. 46 - 51

Physics

Solar Coronal Holes: Solar Activity Cycles

Scientific paper

The distributions of temperature T, density N and velocity V are given using the equations coupling the MHD waves with the coronal atmosphere. It is found that coronal-hole cycle variations of some basic heliospheric parameters, such as V, T and N can be explained by the decrease of the nonradial factor a of the magnetic field in the coronal hole as solar activity is decreased.

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