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

Slides:

Advertisements

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.

Advertisements

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.

– 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.

F1B: Determine the Dominant Processes of Particle Acceleration Phase , Open the Frontier UV Spectroscopic determination of pre/post-shock density,

Current state of the Interhelioprobe mission

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.

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

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.

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.

CopyrightCopyright: NASA Hubble Composite of Pluto.

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.

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.

ILWS and Finland Hannu Koskinen Finland and ILWS2 ILWS science in Finland Finnish Meteorological Institute, Helsinki Magnetospheres.

Solar System Missions Division Solar Orbiter Next major Solar and Heliospheric mission ESA ILWS flagship Now with the Inner Heliospheric Sentinels.

Overview of ERG / ERG Science Center Overview of ERG / ERG Science Center Y. Miyoshi, K. Seki, T. Hori, Y. Miyashita, T. Segawa, Y. Ebihara, T. Takada,

RUSSIAN SPACE MISSIONS FOR SOLAR-TERRESTRIAL SCIENCE ILWS-2011 A.A. Petrukovich, L.M. Zelenyi Space Research Institute V.D. Kuznetsov IZMIRAN.

China National Report , Prague, Czech Republic.

RELEC project (Relativistic ELECtrons). Satellites Low altitudes Geostationary Balloons Arctic Antarctic Ionosphere Atmosphere particles Space and balloon.

ILWS Activities in Hungary K. Kecskemety KFKI RMKI Budapest, Hungary ILWS Steering Committee and Working Group Meeting Prague, June 10–12, 2008.

Stuart D. BaleFIELDS iPDR – Science Requirements Solar Probe Plus FIELDS Instrument PDR Science and Instrument Overview Science Requirements Stuart D.

Aurora, Substorms, and THEMIS D. G. Sibeck NASA/GSFC THEMIS Project Scientist.

Living With a Star Radiation Belt Storm Probes and Associated Geospace Missions D. G. Sibeck Project Scientist NASA Goddard Space Flight Center.

Science - Coronal heating - Coronal structure / dynamics - Elementary processes in Magnetic Reconnection Mission instruments - Optical Telescope / Vector.

1 R U S S I A N F E D E R A T I O N FEDERAL SPACE AGENCY FUNDAMENTAL SPACE RESEARCH WIDE FIELD FOR COOPERATION BETWEEN INDIA AND RUSSIA.

The Solar Orbiter mission Solar Orbiter represents a new approach to solar studies. –A huge increase in discovery space The payload consists of a suite.

29 August, 2011 Beijing, China Space science missions related to ILWS in China

ILWS Activities in Slovakia Karel Kudela IEP SAS Košice, Slovakia ILWS Steering Committee and Working Group Meeting Prague, June 10–12, 2008.

STEREO Planned Launch November, Stereo imaging of Sun; coronal mass ejections from birth to Earth impact. What determines geo-effectiveness of solar.

1 Mars Micro-satellite Mission Japanese micro-satellite mission to Mars to study the plasma environment and the solar wind interaction with a weakly-magnetized.

Solar Orbiter Mission (ESA) - The near-Sun phase  approach the Sun as close as 48 solar radii (~0.22 AU). At these distances, the angular speed of a spacecraft.

Programa de Satélites Científicos e Experimentos do INPE MCE Equatorial Atmosphere Research Satellite Monitor e Imageador de Raios-X Missão Clima Espacial.

The Plasmaspheric Boundary Layer: Some Present-Day Modeling Issues Jan J. Sojka Center for Atmospheric and Space Sciences Utah State University Logan,

THEMIS Workshop 1 UC Berkeley, 18 December 2004 Data Products and Access Tim Quinn UC Berkeley.

Exploitation of Space Ionizing Radiation Monitoring System in Russian Federal Space Agency STRUCTURE OF THE MONITORING SYSTEM The Monitoring System includes.

XVII CLUSTER Workshop, Uppsala, 14 May 2009 Fan and horseshoe instabilities -relation to the low frequency waves registered by Cluster in the polar cusp.

Relating the Equatorward Boundary of the Diffuse Redline Aurora to its Magnetospheric Counterpart Grant, Jeff 1 ; Donovan, Eric 1 ; Spanswick, Emma 1 ;

EGU General Assembly 2006, 2-7 April, 2006, Wien ST6 Multi-point measurements of solar-terrestrial plasma: results and future perspectives Scientific objectives.

Topics in Space Weather Earth Atmosphere & Ionosphere

Space Research Institute Russian magnetospheric & heliospheric missions.

Space Research Institute BMSW - Fast Monitor of Solar Wind Plasma Parameters for current and future missions. M. Riazantseva 1,2, G. Zastenker 1, J. Safrankova.

1 Coronas-F: payload, orbit, performance V. Slemzin CORONAS – Complex ORbital ObservatioNs of Activity of the Sun.

William Liu Canadian Space Agency June 12, 2007, Uppsala, Sweden CSA Report to the 5 th ILWS Working Group Meeting.

Observation of cosmic gamma-ray bursts and solar flares in the ''RELEC'' experiment on the ''VERNOV'' satellite.

Space Weather in Earth’s magnetosphere MODELS  DATA  TOOLS  SYSTEMS  SERVICES  INNOVATIVE SOLUTIONS Space Weather Researc h Center Masha Kuznetsova.

CRRES observations indicate an abrupt increase in radiation belt fluxes corresponding to the arrival of a solar wind shock. The processes(s) which accelerate.

Van Allen Probes Extended Mission Science Themes (1 of 3) 1.Spatial and temporal structures of injections and other transient phenomena and their effects.

Stuart D. BaleFIELDS SOC CDR – Science Requirements Solar Probe Plus FIELDS SOC CDR Science and Instrument Overview Science Requirements Stuart D. Bale.

ILWS, DLR, Dr. Frings ILWS Related Activities in Germany Beijing, August 29, 2011.

European Space Agency, version 1.0, Coordination Group for Meteorological Satellites - CGMS ESA SSA Programme Plans for Space Weather Missions.

Gyeongbok Jo 1, Jongdae Sohn 2, KyeongWook Min 2, Yu Yi 1, Suk-bin Kang 2 1 Chungnam National University 2 Korea Advanced Institute of Science.

Xenon gamma-ray detector for “SIGNAL” experiment

JMA Report on Satellite-based Space Weather Activities in Japan

Connecting Earth to Space: NASA Heliophysics Provides Data on how Space Weather Impacts Earth’s Environment Using NASA Van Allen Probes mission data, researchers.

Kimura, T. , R. P. Kraft, R. F. Elsner, G. Branduardi-Raymont, G. R

Mission overview: two spacecraft that target key radiation belt regions with variable spacing

THEMIS and Space Weather

V. M. Lipunov, E. S. Gorbovskoy

ISAS Solar Physics Yohkoh (1991- ) Hionotori ( )

NASA NASA's Parker Solar Probe mission set off to explore the Sun's atmosphere on Sunday morning August 12, It will swoop to within 4 million miles.

Task Group Report: Ionosphere-Thermosphere

Space activities at Charles University

SWWT Initiatives - Long term monitoring of Sun-Earth Interactions

Presentation transcript:

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

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 km, perigee 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

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 keV ions keV PI: K. Kudela, IEP, w/part DUTH/SSL, IKI Data management system SSNI GB onboard memory possibility of intelligent data handling and compression PI: L. Chesalin, IKI

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

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: ~ km, Perigee: ~ km, Inclination: + and o (two S/C) Co-rotation magnetic tube: up to 3 hours Launch:

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

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 ?

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

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

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 ?

Space Research Institute Microsatellites Kolibri, kg Chibis, 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

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 kg Launch after 2011 Joint IZMIRAN & IKI project

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