How to detect plasmoids in the solar corona?

Details How to detect plasmoids in the solar corona? How to detect plasmoids in the solar corona?

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993achph..66..431n&link_type=abstract

Helvetica Physica Acta, Vol. 66, No. 4, p. 431 - 432

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Scientific paper

The authors examine in a model the movement of closed magnetized structures (plasmoids) in the solar atmosphere. They discuss the development of the ionisation state distributions of oxygen and silicon. Charge states of minor ions are generally important tracers for processes and conditions to which these particles were exposed. In the solar wind they carry information about the inner heliosphere which can otherwise not be derived from other quantities mesurable at 1 AU.

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