Cancellations and structures in the solar photosphere: signature of flares

Details Cancellations and structures in the solar photosphere: signature of flares Cancellations and structures in the solar photosphere: signature of flares

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..695s&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 695-6

Mathematics

Logic

Particle Emission, Solar Wind, Photosphere, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

The topological properties of the typical current structures in a turbulent magnetohydrodynamic flow can be measured using the cancellations analysis. In two-dimensional numerical simulations, this reveals current filaments being the most typical current structures. The observations of the topology of photospheric current structures within active regions shows that modifications occur correspondingly with strong flares.

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