Large-scale emitting chains in the global solar magnetosphere: remarks on cyclical variations

Details Large-scale emitting chains in the global solar magnetosphere: remarks on cyclical variations Large-scale emitting chains in the global solar magnetosphere: remarks on cyclical variations

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.508..387c&link_type=abstract

In: Proceedings of the SOHO 11 Symposium on From Solar Min to Max: Half a Solar Cycle with SOHO, 11-15 March 2002, Davos, Switze

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Solar Large-Scale Chains, Global Solar Magnetosphere, Solar Cycle

Scientific paper

Preliminary remarks on the solar cycle variability of the microwave and EUV large-scale chains are outlined briefly basing on the Nobeyama Radioheliograph and SOHO/EIT data. It is demonstrated that the chains are present in one or another form almost always at all phases of the solar cycle and change their configuration and a character of the emittance during the cycle. The observed complication of the chains in the course of the cycle appears to reflect the corresponding complication of the global solar magnetosphere.

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