Physical Parameters of a Rosette Observed in H-alpha

Details Physical Parameters of a Rosette Observed in H-alpha Physical Parameters of a Rosette Observed in H-alpha

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.29a&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

In May 2002, the solar chromosphere was observed in H? with the two-dimensional 'Gottingen' Fabry-Perot spectrometer which is mounted in the German Vacuum Tower Telescope (VTT) at the Observatorio del Teide/Tenerife. The data consist of broad-band and narrow-band images which were taken by scanning through this line. For a short period of this time series, we calculated the source function, the line-of-sight velocity, the Doppler width and the optical depth using Becker's cloud model. We also estimated the number densities and the temperature of the structure under investigation. Here, we present several results of this study.

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