The TESIS experiment on the CORONAS-PHOTON spacecraft

On February 26, 2009, the first data was obtained in the TESIS experiment on the research of the solar corona using imaging spectroscopy. The TESIS is a part of the scientific equipment of the CORONAS-PHO-TON spacecraft and is designed for imaging the solar corona in soft X-ray and extreme ultraviol...

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Bibliographic Details
Published in:Solar system research 2011-04, Vol.45 (2), p.162-173
Main Authors: Kuzin, S. V., Zhitnik, I. A., Shestov, S. V., Bogachev, S. A., Bugaenko, O. I., Ignat’ev, A. P., Pertsov, A. A., Ulyanov, A. S., Reva, A. A., Slemzin, V. A., Sukhodrev, N. K., Ivanov, Yu. S., Goncharov, L. A., Mitrofanov, A. V., Popov, S. G., Shergina, T. A., Solov’ev, V. A., Oparin, S. N., Zykov, A. M.
Format: Article
Language:English
Subjects:
Altitude
Astronomy
Astrophysics and Astroparticles
Astrophysics and Cosmology
Corona
Imaging
Instrumentation
Management
Observations and Techniques
Physics
Physics and Astronomy
Planetology
Solar corona
Solar flares
Solar physics
Spacecraft
Spectra
Temporal resolution
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Summary:On February 26, 2009, the first data was obtained in the TESIS experiment on the research of the solar corona using imaging spectroscopy. The TESIS is a part of the scientific equipment of the CORONAS-PHO-TON spacecraft and is designed for imaging the solar corona in soft X-ray and extreme ultraviolet regions of the spectrum with high spatial, spectral, and temporal resolutions at altitudes from the transition region to three solar radii. The article describes the main characteristics of the instrumentation, management features, and operation modes.
ISSN:0038-0946
1608-3423
DOI:10.1134/S0038094611020110