AbstractThe images of the solar corona from the limb out to the distance of about 5 solar radii have been obtained for the firs time in the XUV narrow spectral bands and monochromatic lines in the current experiment SPIRIT (). This paper presents the examples of images for the Sun's “quiet” atmosphere as well as for some transient and eruptive events in the corona to illustrate the performance of the instrumentation and to point out the way for future studies. The data obtained will be used for diagnostic purposes and modeling of solar wind acceleration, coronal plasma structures and various active phenomena in the solar corona.
XUV observations of solar corona in the spirit experiment on board the coronas-F satellite
Advances in Space Research ; 32 , 4 ; 473-477
2003-02-28
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
XUV observations of solar corona in the spirit experiment on board the coronas-F satellite
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