Presentation is loading. Please wait.

Presentation is loading. Please wait.

Space Research Institute Future Russian magnetospheric & heliospheric missions L.M. Zelenyi, A.A. Petrukovich, G.N.Zastenker, M.M.Mogilevsky, A.A.Skalsky.

Published byLester Fox Modified over 8 years ago

Similar presentations

Presentation on theme: "Space Research Institute Future Russian magnetospheric & heliospheric missions L.M. Zelenyi, A.A. Petrukovich, G.N.Zastenker, M.M.Mogilevsky, A.A.Skalsky."— Presentation transcript:

1 Space Research Institute Future Russian magnetospheric & heliospheric missions L.M. Zelenyi, A.A. Petrukovich, G.N.Zastenker, M.M.Mogilevsky, A.A.Skalsky Space Research Institute, Russia V.D.Kuznetsov IZMIRAN, Russia Yu. Kotov MEPhI, Russia

2 Space Research Institute Solar-terrestrial payload onboard SPECTR-R SPECTR-R is an international space VLBI project of Russian Space Agency. A 10-meter radio telescope will be launched in late 2008 to an orbit with apogee 350 000 km, perigee 5 000 km inclination 54 o. PLASMA-F is solar-terrestiral payload of opportunity onboard SPECTR-R. Targets:  Fine-scale solar wind, IMF, SCL structures  Solar wind, IMF, SCL monitoring With participation of Slovakia, Czech Rep., Greece, Ukraine, China

3 Space Research Institute PLASMA-F instruments Magnetic field instrument MMFF 2 DC magnetometers 2 AC magnetic sensors (10 Hz – 100 kHz) PI: A. Skalsky, IKI, w/part LSC Fast solar wind monitor BMSW 6 Faraday cups with possibility of instantaneous solar wind velocity vector and density determination PI: G. Zastenker, IKI, w/part ChU, CSS Energetic particle instrument MEP2 geometric factor ~ 1 electrons 15-350 keV ions 15- 3200 keV PI: K. Kudela, IEP, w/part DUTH/SSL, IKI Data management system SSNI-2 200 GB onboard memory possibility of intelligent data handling and compression PI: L. Chesalin, IKI

4 Space Research Institute PLASMA-F features  Synchronized 32 Hz measurements of magnetic field, solar wind ion density, velocity vector, temperature, energetic ions and electrons.  Multi-point solar wind observations with other projects in the frame of ILWS.  1 GByte of data per week  Tests of intelligent onboard data handling Fast-track experiment: decision taken & funding started end of 2004 launch end of 2008 Project Scientist: G.N.Zastenker gzastenk@iki.rssi.ru

5 Space Research Institute Investigation of wave-particle interactions and plasma dynamics in the inner magnetosphere Space Research Institute, Moscow Institute of Applied Physics, N.Novgorod European participation RESONANCE Magnetosynhronous orbit Orbit: Apogee: ~30 000 km, Perigee: ~ 1 800 km, Inclination: + and - 63.4 o (two S/C) Co-rotation magnetic tube: up to 3 hours Launch: 2012 http://resonance.romance.iki.rssi.ru

6 Space Research Institute RESONANCE Magnetospheric science and space weather-related investigations: Ring current and outer radiation belt dynamics Plasmasphere & plasmapause dynamics Sub-auroral zone, auroral zone, polar cap Special task: magnetospheric cyclotron maser observations and active experiments Excitation of waves Modification of precipitation Modification of reflection index at the footprints

7 Space Research Institute RESONANCE Launch 2012: will operate at the same time with Radiation Belt Storm Probes by NASA LWS ERG ORBITALS ILWS inner magnetosphere constellation in 2012 ?

8 Space Research Institute International Space Station electromagnetic environment experiment “Obstanovka” Multipoint multi-component wave and field experiment. Deployment – 2008, by IKI Electro-L: geostationary meteosat, in eastern longitude sector. MeV-range particles KeV-range particles X-ray photometer Magnetometer to be launched in end 2007, Institute of Applied Geophysics, Meteoservice

9 Space Research Institute CORONAS-PHOTON Solar imaging and spectroscopy from EUV to 2000 MeV To be launched in 2008 Moscow Engineering Physics Institute Yu. Kotov http://iaf.mephi.ru

10 Space Research Institute Phobos – Grunt Sample return mission from Phobos Launch 2009 Plasma package onboard: Magnetic field Solar wind ions Planetary ions Multi point heliospheric measurements with STEREO, Messenger ?

11 Space Research Institute Microsatellites Kolibri, 2002 20.5 kg Chibis, 2008 40 kg  IKI design and manufacturing  Launch in LEO orbit from a space station or piggy-back Scientific tasks: Ionospheric monitoring: plasma and wave measurements CO2 and atmosphere composition Med-resolution surface imaging Educational programs

12 Space Research Institute Solar Instrumentation Optical telescope Magnetograph X-ray imager-spectrometer Coronagraph INTERHELIOPROBE: heliospheric mission with perihelion 30 Rs After 2012 Heliospheric instrumentation Solar wind ion, electron analyzer Dust analyzer Magnetic, wave and radio instrument Energetic particle telescope Neutron detector Payload 50-60 kg Launch after 2011 Joint IZMIRAN & IKI project

13 Space Research Institute Mini-spacecraft for magnetospheric science Currently under development, first launch of the platform in 2008 Possible collaboration with future MMS / X-scale projects Sci payload weight ~ 40 kg

Download ppt "Space Research Institute Future Russian magnetospheric & heliospheric missions L.M. Zelenyi, A.A. Petrukovich, G.N.Zastenker, M.M.Mogilevsky, A.A.Skalsky."

Similar presentations

1 Kuafu A mission to start a mission William Liu Canadian Space Agency & Chinese Academy of Sciences August 29, 2011, 3rd ILWS Science Symposium, Beijing.

1 Kuafu A mission to start a mission William Liu Canadian Space Agency & Chinese Academy of Sciences August 29, 2011, 3rd ILWS Science Symposium, Beijing.
Workshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”, 6 – 8 December 2005, Wrocław Spectroscopy Department.

Workshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”, 6 – 8 December 2005, Wrocław Spectroscopy Department.
Future Plans for Space Weather Observations – U.S. NOAA Perspective Terry Onsager National Oceanic and Atmospheric Administration Space Weather Prediction.

Future Plans for Space Weather Observations – U.S. NOAA Perspective Terry Onsager National Oceanic and Atmospheric Administration Space Weather Prediction.
– Ukrainian input in ILWS program O. FEDOROV Institute of Space Research, Kyiv, Ukraine V. KOREPANOV Lviv Centre of Institute of Space Research, Lviv,

– Ukrainian input in ILWS program O. FEDOROV Institute of Space Research, Kyiv, Ukraine V. KOREPANOV Lviv Centre of Institute of Space Research, Lviv,
From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.

From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.
F1B: Determine the Dominant Processes of Particle Acceleration Phase 2005-2015, Open the Frontier UV Spectroscopic determin- ation of pre/post-shock density,

F1B: Determine the Dominant Processes of Particle Acceleration Phase , Open the Frontier UV Spectroscopic determin- ation of pre/post-shock density,
Current state of the Interhelioprobe mission

Current state of the Interhelioprobe mission
International Colloquium and Workshop Ganymede Lander: scientific goals and experiments

International Colloquium and Workshop "Ganymede Lander: scientific goals and experiments"
Solar Probe: Mission to the Sun Donald M. Hassler/David J. McComas Southwest Research Institute.

Solar Probe: Mission to the Sun Donald M. Hassler/David J. McComas Southwest Research Institute.
Stuart D. BaleFIELDS iCDR – Science Requirements Solar Probe Plus FIELDS Instrument CDR Science and Instrument Overview Science Requirements Stuart D.

Stuart D. BaleFIELDS iCDR – Science Requirements Solar Probe Plus FIELDS Instrument CDR Science and Instrument Overview Science Requirements Stuart D.
1 Future solar missions (Based on the summary by R.A. Harrison) S. Kamio 2004.11.15.

1 Future solar missions (Based on the summary by R.A. Harrison) S. Kamio
Österreichische Akademie der Wissenschaften (ÖAW) / Institut für Weltraumforschung (IWF), Graz, Austria, T +43/316/4120-400, iwf.oeaw.ac.atDownload:2013.

Österreichische Akademie der Wissenschaften (ÖAW) / Institut für Weltraumforschung (IWF), Graz, Austria, T +43/316/ , iwf.oeaw.ac.atDownload:2013.
RESONANCE Project for Studies of Wave-Particle Interactions in the Inner Magnetosphere Anatoly Petrukovich and Resonance team RESONANCEРЕЗОНАНС R.

RESONANCE Project for Studies of Wave-Particle Interactions in the Inner Magnetosphere Anatoly Petrukovich and Resonance team RESONANCEРЕЗОНАНС R.
The Sun and the Heliosphere: some basic concepts…

The Sun and the Heliosphere: some basic concepts…
Solar Orbiter. Contents The mission The mission The orbit The orbit The instruments The instruments VIM: Visible-light Imager and Magnetograph VIM: Visible-light.

Solar Orbiter. Contents The mission The mission The orbit The orbit The instruments The instruments VIM: Visible-light Imager and Magnetograph VIM: Visible-light.
CopyrightCopyright: NASA Hubble Composite of Pluto.

CopyrightCopyright: NASA Hubble Composite of Pluto.
RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.

RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.
Brief introduction of YINGHUO-1 Micro-satellite for Mars environment exploration J. Wu, G. Zhu, H. Zhao, C. Wang, L. Lei, Y. Sun, W. Guo and S. Huang Center.

Brief introduction of YINGHUO-1 Micro-satellite for Mars environment exploration J. Wu, G. Zhu, H. Zhao, C. Wang, L. Lei, Y. Sun, W. Guo and S. Huang Center.
THE STUDY OF ELECTROMAGNETIC PARAMETERS OF SPACE WEATHER Thunderstorms and Elementary Particle Acceleration (TEPA-2010) MICRO-SATELLITE “CHIBIS- M”

THE STUDY OF ELECTROMAGNETIC PARAMETERS OF SPACE WEATHER Thunderstorms and Elementary Particle Acceleration (TEPA-2010) MICRO-SATELLITE “CHIBIS- M”
Solar Probe Plus A NASA Mission to Touch the Sun Solar Probe Plus – A Mission to Touch the Sun Rob Decker and Nicky Fox Johns Hopkins Applied Physics Laboratory.

Solar Probe Plus A NASA Mission to Touch the Sun Solar Probe Plus – A Mission to Touch the Sun Rob Decker and Nicky Fox Johns Hopkins Applied Physics Laboratory.

Similar presentations

Ads by Google