principle investigator: dr. yu.d. kotov tel/fax (007-095)-3240616 e-mail: [email protected]
DESCRIPTION
Launch date: end of 2007, from Plesetsk (Russia). Space Research Program. RUSSIAN SATELLITE PROJECT "CORONAS-PHOTON" FOR THE STUDY OF SOLAR FLARE HARD RADIATIONS. Russian Aviation and Space Agency Russian Academy of Science Principal Organization: Moscow Engineering Physics Institute. - PowerPoint PPT PresentationTRANSCRIPT
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Principle Investigator: Dr. Yu.D. KotovTel/fax (007-095)-3240616E-mail: [email protected]
Space Research Program
RUSSIAN SATELLITE PROJECTRUSSIAN SATELLITE PROJECT"CORONAS-PHOTON""CORONAS-PHOTON"
FOR THE STUDY OF SOLAR FLARE FOR THE STUDY OF SOLAR FLARE HARD RADIATIONSHARD RADIATIONS
Russian Aviation and Space AgencyRussian Academy of Science
Principal Organization: Moscow Engineering Physics Institute
Launch date: end of 2007, from Plesetsk (Russia)
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
CORONAS-PHOTON mission is the third satellite of the Russian CORONAS program on the Solar activity observations. The main goal of the CORONAS-PHOTON mission is the study of the Solar flare hard electromagnetic radiation in the wide energy range from Extreme UV up to high energy gamma - radiation (~2000MeV).
It is adopted as a part of the Russian Federal Program of Fundamental Space Researches. The project is a part of International Living With the Star (ILWS) program.
Goal of the project: Investigation of the process of energy accumulation and its
transformation to the energy of accelerated particles during solar flares, study of the acceleration mechanisms, propagation and interaction of the fast particles in the solar atmosphere.
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Direct solar flare radiation
Study of the temporal dynamic of hard electromagnetic radiation from full disk in a wide energy range from EUV to 2000MeV;
Study of spatial and temporal dynamics of hot plasma regions in Solar atmosphere by observation of X- ray/XUV radiation;
XUV full Sun spectroscopy;Nuclear gamma-lines spectroscopy of Solar activity regions;Detection of solar neutrons with energies higher 20MeV;Measurement of linear polarization and rapid variability of hard X-ray emission during the flares;
•Monitoring of the Solar extreme ultra-violet (EUV), soft and hard X-ray emissions;
Main objectives of the mission
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
CORONAS-PHOTON mission scientific Payload:1. High energy radiation spectrometer NATALYA Gamma-rays spectroscopy 0.3 –
2000MeV;Neutrons 20 – 300MeV
2. Low energy gamma-ray spectrometer RT - 2 Phoswich mode: 15 – 150keV; Spectrometric mode: 100 – 2000keV
3. Hard X-ray polarimeter PENGUIN-M (X-ray radiation 1 – 10keV; X-ray polarization 20 – 150keV; X-ray & gamma-ray spectroscopy 0.15 – 5MeV)
4. Fast X-ray monitor FXM (Hard X-ray with sub-msec temporal resolution 20 – 500keV )
5. Solar flare and cosmic gamma-burst spectrometer KONUS-RF (Hard X-ray & gamma-ray spectroscopy with high temporal resolution (0.0112)MeV )
6. XUV TeleScope/ Imaging Spectrometer TESIS
7. Multi-channel Extreme ultra-violet and Soft X-ray monitor PHOKA (Timing of the full disk radiation in 7 spectral windows from 10nm to visual band )
8. Energetic particle analyzer ELECTRON-M-PESCA (e : 0.2 – 2MeV p : 1.0 – 150MeV α : 1.5 – 50MeV/nucleon Nuclei (Z <26) 2.0 – 50MeV/nucleon )
9. Energetic particle telescope STEP-F (e : 0.15 – 10MeV p : 4.0 – 62MeV α : 15.5 – 245.5MeV )
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Orbit and LauncherOrbit and Launcher Circular 500 km; Period 95 min (60 min Sun/orbit)Circular 500 km; Period 95 min (60 min Sun/orbit) Orbit inclination 82°5 ; 2 weeks/ 3 months full Sun orbitsOrbit inclination 82°5 ; 2 weeks/ 3 months full Sun orbits
Launcher: Cyclon-3MLauncher: Cyclon-3M Launching date 2007Launching date 2007
Lifetime 3 –5 yearsLifetime 3 –5 years
Weight satellite: 1900 kg;Weight satellite: 1900 kg; scientific payload: 540 kg scientific payload: 540 kg
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Overview of TESIS instrumentsOverview of TESIS instruments
The main emitting ions and wavelengthsThe main emitting ions and wavelengths
Ion Wavelength, Å T, ºKHeII 304,8 5*104
SiXI 304.3 1.6*106
FeVIII-FeXX 132; 1. & 12*106 MgXII 8.418; 8.423 (1-2)*107
Spectroheliograms 280 to 330 (0.05- 12)*106
The goal of the experiment “TESIS” is to study the structure and the dynamics of the solar atmosphere over a broad range of heights
and temperatures using full sun XUV spectroscopic imaging.Lebedev Physical Institute of the Russian Academy of Sciences
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Main parameters of TESIS channelsMain parameters of TESIS channels
Name of channel
Parameter
FeXX (XUV
telescope)
HeII (XUV
telescope-coronagraph)
WF (XUVwide field
telescope-coronagraph)
Mg XII (spectro-
heliometer)
XUV spectro-heliometer
SphinX Solar
Photometer in X-rays
Spectral band, Å 131-133 295-315 8.418-8.423 280-335 1- 10 keV Field of view Full disk: 60 60 in the
field of 2.5 Corona up to 5
radii - 2.5 Full disk: 60
1.6 (cross to dispertion)
Spatial resolution, arcsec
1,7 4.4 2 3 (cross to dispertion)
256 channel
Spectral resolution
/~70 /~20 /~20 2*10-4 Å/pix 2*10-2 Å/pix Full Sun
Exposure time/ temporal resolution, sec
0.01 – 600 / up to 0.5 100 Hz-1000 Hz
Principal optical element
Off-axis paraboloid, Multi-layer coating
Ritchey-Chrétien 2 mirror system,
Multi-layer coating
Bragg spherical crystal quartz
Diffraction grating with 3600
l/mm
Detector backside CCD42-40 AIMO by E2V (2Kx2K size , 13.5x13.5 um), with Peltier cooler, similar to CCDs used in Secchi of Stereo
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Artificial moon
Entrance filter
Detector
132A 304A
Shutter
Multilayer mirror
Pointing and focusing mechanism
Optical layout of the XUV telescopes of TESIS instrument
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Wide field EUV Telescope:
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
synthetic quartz 2d=8.501 A 80x120 mm
MgXII spectrogeliograph
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Typical image given by the spectroheliograph
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Deep spectroheliogram to show a large extension of 304 emissions
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
SphinX Solar Photometer in X-ray
PI – Janusz Sylwester SRC PAS
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Main features of the TESIS experiment Full disk spectroscopic imaging: 4 EUV channels 1 MgXII channels Simultaneous observations in all spectral channels Temporal resolution up to 0.5 sec XUV observations of the corona, up to 5 solar radius Full Sun spectroheliograms in 280- 330 A Ritchey-Chrétien Wide FOV 304 telescope SphinX Solar Photometer in X-rays
Study of the upper Earth atmosphere Observation of space debris
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
On board computing and data collection features
• 50MIPS DSP• 128MB data RAM• Up to 4 Ch. Simultaneously + SphinX• 8 sec readout time (2Kx2K image)• Update on board S/W• Loose less data compression algorithm (c.r. 2-4)• JPEG like data compression algorithm (c.r. 10-???)• 500 MB/day data rate
WorkshopWorkshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”RHESSI and SPIRIT Instruments”, , 6 – 8 December 20056 – 8 December 2005, , WrocławWrocław
Spectroscopy DepartmentSpectroscopy DepartmentLebedev Physical InstituteLebedev Physical InstituteMoscowMoscow
Coronas-Photon doing electrical tests at MEPhI Sept 2005
TESIS