Flows, Boundaries, Interactions

Details Flows, Boundaries, Interactions Flows, Boundaries, Interactions

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..934.....d&link_type=abstract

Flows, Boundaries, and Interaction Workshop; Cristiana Dumitrache, Astronomical Institute of the Romanian Academy, Bucharest, Ro

Astronomy and Astrophysics

Astronomy

Magnetohydrodynamics And Plasmas, Electric And Magnetic Fields, Solar Magnetism

Scientific paper

Observations in chromospheric lines and the visible continuum together with photospheric helio-seismic measurements make possible to image a 3-dimensional profile of a sun quake in a flaring region. Chromospheric line observations show us the part of the solar atmosphere where high-energy electrons are thought to cause thick target heating that then could also cause intense white-light emission and could drive seismic waves into the active region subphotosphere. we present here the preliminary results of the sun quake of July 16, 2004.

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