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TESIS experiment on XUV imaging spectroscopy of the Sun onboard the CORONAS-PHOTON satellite

Published online by Cambridge University Press:  01 November 2006

S.V. Kuzin
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
I.A. Zhitnik
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
S.A. Bogachev
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
S.V. Shestov
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
O.I. Bugaenko
Affiliation:
P.K. Sternberg Astronomical Institute, Moscow State University, Russia email: [email protected]
N.K. Suhodrev
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
A.A. Pertsov
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
A.V. Mitrofanov
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
A.P. Ignat'ev
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
V.A. Slemzin
Affiliation:
P.N. Lebedev Physical Institute of Russian Academy of Science, Russia email: [email protected]
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Abstract

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We present a brief description of new complex of space telescopes and spectrographs, TESIS, which will be placed aboard the CORONAS-PHOTON satellite. The complex is intended for high-resolution imaging observation of full Sun in the coronal spectral lines and in the spectral lines of the solar transition region. TESIS will be launched at the end of 2007 – early of 2008. About 25 % of the daily TESIS images will be free for use and for downloading from the TESIS data center that is planned to open 2 months before the TESIS launching at http://www.tesis.lebedev.ru

Type
Contributed Papers
Copyright
© 2006 International Astronomical Union