Chromospheric Line Emission Analysis of the July 16, 2004 Sun Quake

Details Chromospheric Line Emission Analysis of the July 16, 2004 Sun Quake Chromospheric Line Emission Analysis of the July 16, 2004 Sun Quake

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..934...38b&link_type=abstract

FLOWS, BOUNDARIES, INTERACTIONS: Flows, Boundaries, and Interaction Workshop. AIP Conference Proceedings, Volume 934, pp. 38-43

Physics

1

Helioseismology, Pulsations, And Shock Waves, Flares, Chromosphere

Scientific paper

Observations in chromospheric lines and the visible continuum together with photospheric helioseismic 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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