KORTES Mission for Solar Activity Monitoring Onboard International Space Station

被引:6
作者
Kirichenko, Alexey [1 ]
Kuzin, Sergey [1 ]
Shestov, Sergey [1 ,2 ]
Ulyanov, Artem [1 ]
Pertsov, Andrey [1 ]
Bogachev, Sergey [1 ]
Reva, Anton [1 ]
Loboda, Ivan [1 ]
Vishnyakov, Eugene [1 ]
Dyatkov, Sergey [1 ]
Erkhova, Nataliya [1 ]
Steslicki, Marek [3 ]
Sylwester, Janusz [3 ]
Plocieniak, Stefan [3 ]
Podgorski, Piotr [3 ]
Kowalinski, Miroslaw [3 ]
Bakala, Jaroslaw [3 ]
Szaforz, Zaneta [3 ]
Siarkowski, Marek [3 ]
scislowski, Daniel [3 ]
Mrozek, Tomasz [3 ]
Sylwester, Barbara [3 ]
Malyshev, Ilya [4 ]
Pestov, Alexey [4 ]
Polkovnikov, Vladimir [4 ]
Toropov, Mikhail [4 ]
Salashchenko, Nikolay [4 ]
Tsybin, Nikolay [4 ]
Chkhalo, Nikolay [4 ]
机构
[1] Russian Acad Sci, PN Lebedev Phys Inst, Opt Dept, Lab Xray Astron Sun, Moscow, Russia
[2] Royal Observ Belgium, Solar Terr Ctr Excellence IDC, Brussels, Belgium
[3] Polish Acad Sci, Space Res Ctr, Warsaw, Poland
[4] Russian Acad Sci, Inst Phys Microstruct, Nizhnii Novgorod, Russia
关键词
solar corona; solar flares; polarimetry; spectroscopy; solar imaging; extreme ultraviolet; soft X-rays; international space station; CORONAL MASS EJECTIONS; EXTREME-ULTRAVIOLET; PLASMA STRUCTURES; EUV; SPECTROHELIOGRAPH; MICROFLARES; RECONNECTION; NANOFLARES; INITIATION; EVOLUTION;
D O I
10.3389/fspas.2021.646895
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a description of the recent advances in the development of the KORTES assembly-the first solar oriented mission designed for the Russian segment of the International Space Station. KORTES consists of several imaging and spectroscopic instruments collectively covering a wide spectral range extending from extreme ultraviolet (EUV) wavelengths to X-rays. The EUV telescopes inside KORTES will trace the origin and dynamics of various solar phenomena, e.g., flares, CMEs, eruptions etc. EUV spectra provided by grazing-incidence spectroheliographs will enable precise DEM-diagnostics during these events. The monochromatic X-ray imager will observe the formation of hot plasma in active regions and outside them. The SolpeX module inside KORTES will offer an opportunity to measure fluxes, Doppler shifts and polarization of soft X-ray emission both in lines and continuum. SolpeX observations will contribute to studies of particle beams and chromospheric evaporation. The instrumentation of KORTES will employ a variety of novel multilayer and crystal optics. The deployment of KORTES is planned for 2024.
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页数:11
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