Space Research Institute Russian magnetospheric & heliospheric missions.

Slides:

Advertisements

Similar presentations

COSPAR E July 22, Paris revised for Nobeyama Symposium 2004 October 29, Kiyosato Takeo Kosugi (ISAS/JAXA, Japan)

Advertisements

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.

Flare Luminosity and the Relation to the Solar Wind and the Current Solar Minimum Conditions Roderick Gray Research Advisor: Dr. Kelly Korreck.

Earth’s Radiation Belt Xi Shao Department of Astronomy, University Of Maryland, College Park, MD

From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.

Solar system science using X-Rays Magnetosheath dynamics Shock – shock interactions Auroral X-ray emissions Solar X-rays Comets Other planets Not discussed.

DOPPLER DOPPLER A Space Weather Doppler Imager Mission Concept Exploration Science Objectives What are the most relevant observational signatures of flare,

Magnetospheric Morphology Prepared by Prajwal Kulkarni and Naoshin Haque Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global.

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

Geospace Variability through the Solar Cycle John Foster MIT Haystack Observatory.

International Colloquium and Workshop "Ganymede Lander: scientific goals and experiments"

Tuija I. Pulkkinen Finnish Meteorological Institute Helsinki, Finland

Solar Probe: Mission to the Sun Donald M. Hassler/David J. McComas Southwest Research Institute.

Österreichische Akademie der Wissenschaften (ÖAW) / Institut für Weltraumforschung (IWF), Graz, Austria, T +43/316/ , iwf.oeaw.ac.atDownload:2013.

Seminar in association with the MEDOC 12 campaign, Nov 2003 Solar Orbiter Work of the ESA/NASA Solar Orbiter Study Team Presented by Alan Gabriel, IAS.

RESONANCE Project for Studies of Wave-Particle Interactions in the Inner Magnetosphere Anatoly Petrukovich and Resonance team RESONANCEРЕЗОНАНС R.

Hinode: A New Solar Observatory in Space H. Hara ( NAOJ/NINS) and the Hinode team 2007 Dec 8.

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.

Radiation conditions during the GAMMA-400 observations:

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.

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.

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.

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.

195 Å image – behind 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – Sun- Earth line – SOHO/ EIT image 195 Å image – ahead SECCHI Extreme.

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.

China National Report , Uppsala, Sweden China National Space Administration.

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

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.

Space Science MO&DA Programs - September Page 1 SS It is known that the aurora is created by intense electron beams which impact the upper atmosphere.

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

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

Nishu Karna Mentor:Dr. William Dean Pesnell Code: 671 SESI Program-2009 Goddard Space Flight Center St. Cloud State University Date: August 5, 2009 RELATIVISTIC.

Particle Transport in the Heliosphere: Part 1 Gaetano Zimbardo Universita’ della Calabria, Cosenza, Italy with contributions from S. Perri, P. Pommois,

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.

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

Radiation Storms in the Near Space Environment Mikhail Panasyuk, Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University.

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

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

Preliminary Presentation By Matthew Lewis 2 nd December 2005.

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.

한 미 려 – Introduction (1) 2.Instrument & Observe 3.Science 2.

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

Solar and heliosheric WG

Solar Probe Plus Scheduled to be launched in 2018 Solar Probe Plus will come closer to the Sun than any spacecraft has ever flown - and what it finds could.

THEMIS and Space Weather

ISAS Solar Physics Yohkoh (1991- ) Hionotori ( )

NASA Nasa's Parker Solar Probe mission set off to explore the Sun's atmosphere in the summer of The probe will swoop to within 4 million miles of.

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.

Introduction to Space Weather

Space activities at Charles University

Transition Region and Coronal Explorer (TRACE)

SWWT Initiatives - Long term monitoring of Sun-Earth Interactions

Richard B. Horne British Antarctic Survey Cambridge UK

Presentation transcript:

Space Research Institute Russian magnetospheric & heliospheric missions

Space Research Institute CORONAS-PHOTON Solar imaging and spectroscopy from EUV to 2000 MeV To be launched in fall 2008 Moscow Engineering Physics Institute Yu. Kotov Currently flight payload is delivered. Completion of satellite Preparation is expected in August

Space Research Institute Solar-terrestrial payload onboard SPECTR-R space VLBI project. 10-meter radio telescope orbit with apogee km launch in late 2008 or 2009 Currently main flight payload is under integration test PLASMA-F is solar-terrestiral payload of opportunity onboard SPECTR-R. will be delivered after competion of main payload tests. Targets: Fine-scale solar wind, IMF, SCL up to 32 samples/sec Solar wind, IMF, SCL monitoring Project Scientist: G.N.Zastenker

Space Research Institute PLASMA-F instruments Magnetic field instrument MMFF – Russia 2 DC magnetometers 2 AC magnetic sensors (10 Hz – 100 kHz) PI: A. Skalsky, IKI, w/part LSC Fast solar wind monitor BMSW - Czech R., China 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 – Slovakia, Greece geometric factor ~ 1 electrons keV ions keV PI: K. Kudela, IEP, w/part DUTH/SSL, IKI Data management system SSNI-2 – Russia 100 GB onboard memory possibility of intelligent data handling and compression PI: L. Chesalin, IKI

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 Apogee: ~ km, Perigee: ~ km, Inclination: + and o (two S/C) Co-rotation magnetic tube: up to 3 hours Launch: 2012 on schedule Currently change from 2x300 kg to 4x150 kg satellites is considered.

Space Research Institute RESONANCE 2А и 2В RESONANCE 1А и 1В ~ 1-10 km ~ ~

Space Research Institute RESONANCE Space weather-related Ring current and outer radiation belt dynamics Plasmasphere & plasmapause dynamics Magnetospheric cyclotron maser Auroral region processes Interaction of electrons and waves small scale acceleration zones

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

Space Research Institute Small satellite platform KARAT for scientific projects Dry weight ~ 100 kg plus up to 60 kg of payload First launch in 2009 Later used in Resonance, etc

Space Research Institute Mini-spacecraft for magnetospheric science Possible collaboration with future MMS / X-scale projects Sci payload weight ~ 40 kg

Space Research Institute MAIN SCIENTIFIC GOALS mechanisms of the coronal heating and solar wind fine structure and dynamics of the solar atmosphere origin and the global dynamics of solar flares and CMEs generation and propagation of solar energetic particles mechanism of the solar dynamo and solar cycle high latitudes studies Interhelioprobe Launch In fall 2008 decision to start phase B will be taken.

Space Research Institute Start from the Earth INTERHELIOPROBE Multiple Venus Flight-by Inclination of the orbit

Space Research Institute INTERHELIOPROBE High resolution observations Fine structure and dynamics of solar atmosphere: magnetic network; magnetic flux elements; turbulence. Supergranulation and its role in large-scale dynamics of magnetic field and corona Small-scale magnetic activity: loops dynamics and motions of its footpoints, microflares, reconnection.

Space Research Institute INTERHELIOPROBE In - situ measurements near the Sun Distribution function. Remnants of coronal heating and related plasma processes. Wave-particle interactions. Beams. Temperature anisotropy. Radio emission. Neutrons.

Space Research Institute SOLAR INSTRUMENTATION Optical telescope Magnetograph X-ray imager-spectrometer Coronograph HELIOSPHERIC INSTRUMENTATION Solar Wind Ion Analyzer Solar Wind Electron Analyzer Solar Wind Plasma and Dust Analyzer Magnetic Wave Complex Magnetometer Energetic Particle Telescope Neutron Detector Radio Spectrometer Detector Mass: 100 kg  Power: 100 W  Telemetry: 100 kb/s INTERHELIOPROBE

Space Research Institute INTERHELIOPROBE in Aphelion

Space Research Institute A joint IZMIRAN & IKI Project Contact: Prof. Kuznetsov, IZMIRAN Interhelioprobe & Solar Orbiter RSA & ESA 2014