Note on the problem of physics of chromospheric cavities.

Details Note on the problem of physics of chromospheric cavities. Note on the problem of physics of chromospheric cavities.

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989bsold..11..107b&link_type=abstract

Byulletin Solnechnye Dannye Akademie Nauk USSR, No. 1989/811 p. 107 - 111

Physics

Solar Chromosphere: Instabilities, Solar Chromosphere: Physics

Scientific paper

It is shown that the radial motion of matter in Hα is predominantly directed to the solar surface in rarified regions of the chromosphere (chromospheric cavities). The velocity of lowering of matter is of the order of 1 km/sec. A conception is developed that chromospheric cavities are rarified regions with a nearly zero intensity of the magnetic field. As a result thermal instability takes place in the corona and the upper chromosphere.

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