Wrocław in Space: X-ray Diagnostics of Solar Corona

Details Wrocław in Space: X-ray Diagnostics of Solar Corona Wrocław in Space: X-ray Diagnostics of Solar Corona

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..812..393s&link_type=abstract

PLASMA 2005: Int. Conf. on Research and Applications of Plasmas; 3rd German-Polish Conf.on Plasma Diagnostics for Fusion and App

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Corona, X-Ray

Scientific paper

X-ray observations of the solar corona have been undertaken in Solar Physics Division (Space Research Centre of the Polish Academy of Sciences, Wrocław) for more than 35 years. Short history of these observations is presented. We focus mainly on the results from the latest experiments. These are hard X-ray photometer onboard the INTERBALL-Tail Probe and two Bragg crystal spectrometers recording solar X-ray spectra from CORONAS-F satellite. Such observations provide useful information on solar coronal plasma heated up to temperatures of several 106 - 107 K.

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