Author/Authors :
I. Zhitnik، نويسنده , , S. Kuzin، نويسنده , , A. A. Afanasev، نويسنده , , O. Bugaenko، نويسنده , , A. Ignatev، نويسنده , , V. Krutov، نويسنده , , A. Mitrofanov، نويسنده , , S. Oparin، نويسنده , , A. Pertsov، نويسنده , , V. Slemzin، نويسنده , , N. Sukhodrev، نويسنده , , A. Umov، نويسنده ,
Abstract :
The 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 (SPectroheliographIc soft X-Ray Imaging Telescope). This paper presents the examples of images for the Sunʹs “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.
