Relation between solar surface and coronal processes - simulations and spacecraft observations

Details Relation between solar surface and coronal processes - simulations and spacecraft observations Relation between solar surface and coronal processes - simulations and spacecraft observations

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009eguga..11.3435b&link_type=abstract

"EGU General Assembly 2009, held 19-24 April, 2009 in Vienna, Austria http://meetings.copernicus.org/egu2009, p.3435"

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Ongoing HINODE and STEREO spacecraft observations provide better than ever information about the processes occuring at the solar surface and those in the solar corona as well as in the heliosphere. Numerical simulations are necessary to verify their possible causual relationship. We review appropriate modelling approaches able to describe major coupling effects between the photosphere, the chromosphere and the outer atmosphere of the Sun in comparison with HINODE and STEREO spacecraft observations. In particular we draw attention at toplogical features and at the evolution of the magnetic helicity and preceeding eruptions of Flares and CMEs.

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