The TESIS experiment on the CORONAS-PHOTON spacecraft
| Autor: | N. K. Sukhodrev, S. N. Oparin, T. A. Shergina, Yu. S. Ivanov, A. A. Pertsov, Sergey A. Bogachev, L. A. Goncharov, S. G. Popov, A. M. Zykov, A. A. Reva, A. V. Mitrofanov, S. V. Shestov, I. A. Zhitnik, Sergey Kuzin, V. A. Solov’ev, A. S. Ulyanov, Vladimir Slemzin, O. I. Bugaenko, A. P. Ignat'ev |
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| Rok vydání: | 2011 |
| Předmět: |
Physics
Photon Spacecraft business.industry Astrophysics::High Energy Astrophysical Phenomena Instrumentation Astronomy Astronomy and Astrophysics Solar radius Imaging spectroscopy Optics Planetary science Space and Planetary Science Extreme ultraviolet Physics::Space Physics Extreme ultraviolet Imaging Telescope Astrophysics::Solar and Stellar Astrophysics Astrophysics::Earth and Planetary Astrophysics business |
| Zdroj: | Solar System Research. 45:162-173 |
| ISSN: | 1608-3423 0038-0946 |
| DOI: | 10.1134/s0038094611020110 |
| Popis: | 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. |
| Databáze: | OpenAIRE |
| Externí odkaz: |
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