Update of the French activities relevant to ILWS

Slides:



Advertisements
Similar presentations
The Science of Solar B Transient phenomena – this aim covers the wide ranges of explosive phenomena observed on the Sun – from small scale flaring in the.
Advertisements

Space Weather Observations from the GOLD Mission Richard Eastes and the GOLD Team ( W. E. McClintock, A. G. Burns, S. C. Solomon, D. N. Anderson, L. Andersson,
COSPAR E July 22, Paris revised for Nobeyama Symposium 2004 October 29, Kiyosato Takeo Kosugi (ISAS/JAXA, Japan)
Geospace Electrodynamic Connections (GEC) Mission The GEC mission has been in the formulation phase as part of NASA’s Solar Terrestrial Probe program for.
Workshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”, 6 – 8 December 2005, Wrocław Spectroscopy Department.
ISRO Update Dr. Jayati Datta Programme Manager, Chandrayaan-1 Programme Manager, Space Science Office ISRO HQ Antariksh Bhavan New BEL Road Bangalore 560.
1 TARANIS - a satellite project dedicated to the physics of TLEs and TGFs F. Lefeuvre 1, E. Blanc 2, J.L. Pinçon 1 and the TARANIS team* 1 LPCE /CNRS –
Terrestrial Gamma-ray Flashes. Gamma Ray Astronomy Beginning started as a small budget research program in 1959 monitoring compliance with the 1963 Partial.
MSU Space Project «Lomonosov». MSU Space Project «Lomonosov» Participants of the experiment (preliminary list): M.V. Lomonosov Moscow State University.
CNES has scheduled the launch of PICARD microsatellite in October (1) SA (F) IRMB (B) PMOD (Ch) OCA Nice University IAS LMD (3) Yale university HAO.
From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.
SDO Project Science Team 1 The Science of SDO. SDO Project Science Team 2 Sensing the Sun from Space  High-resolution Spectroscopy for Helioseismology.
TARANIS a CNES Scientific Mission – C. Bastien-Thiry Workshop on Coupling of Thunderstorms and Lightning Discharges to Near-Earth Space – Corte 2008 TARANIS.
Solar-B/EIS high-cadence observation for diagnostics of the corona and TR S. Kamio (Kyoto Univ.) Solar-B domestic meeting.
1 Future solar missions (Based on the summary by R.A. Harrison) S. Kamio
Hinode: A New Solar Observatory in Space H. Hara ( NAOJ/NINS) and the Hinode team 2007 Dec 8.
Enabling Technology Development: High cadence imaging spectrograph development Low mass/power instrumentation Advanced communication/DSN for future deployment.
CROSS-SCALE and SCOPE: The future in Space Plasma Physics Matt Taylor on behalf of Steve Schwartz, Masaki Fujimoto and the Cross-Scale and SCOPE Teams.
RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.
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.
Update of the French activities relevant to ILWS Jean-Yves Prado, CNES.
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.
Solar Wind and Coronal Mass Ejections
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.
The Sun.
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.
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.
NCKU UCB Tohoku ISUAL / ROCSAT-2 August 2001 Sprites observation by ISUAL on the ROCSAT-2 satellite J. L. Chern, R. R. Hsu, H. T. Su, A. B. Chen, and L.
Solar space-born instruments and detectors for X-ray observations of the solar corona. Szymon Gburek Space Research Centre Polish Academy of Sciences,
Programa de Satélites Científicos e Experimentos do INPE MCE Equatorial Atmosphere Research Satellite Monitor e Imageador de Raios-X Missão Clima Espacial.
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.
Space Research Institute Future Russian magnetospheric & heliospheric missions L.M. Zelenyi, A.A. Petrukovich, G.N.Zastenker, M.M.Mogilevsky, A.A.Skalsky.
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.
ISUAL Design Concept S. Mende. SDR 7 Jun NCKU UCB Tohoku ISUAL Design Concept S. Mende Sprite Example Sprite Image obtained by Berkeley/NCKU 1999.
The Sun Created by the Lunar and Planetary Institute For Educational Use Only LPI is not responsible for the ways in which this powerpoint may be used.
한 미 려 – Introduction (1) 2.Instrument & Observe 3.Science 2.
KMA Space Weather Service Presented to CGMS-44 on Working Group SWTT.
for Lomonosov-GRB collaboration
Xenon gamma-ray detector for “SIGNAL” experiment
NOAA L1 Status and Studies
Focal Plane Instrumentation at Big Bear Solar Observatory
Solar and heliosheric WG
European Space Weather Week - 13
A joint study of the University of Göttingen (1) and Astrium (2)
The Solar Oblateness Measured On Board The PICARD Spacecraft,
Solar Dynamics Observatory (SDO)
THEMIS and Space Weather
Upcoming Facilities of IIA
The ionosphere is much more structured and variable than ever predicted. Solar Driven Model Since 2000, we have seen more, very clear evidence that the.
R. Bucˇık , K. Kudela and S. N. Kuznetsov
V. M. Lipunov, E. S. Gorbovskoy
Space Weather Activities in China
Gérard Thuillier, Service d’Aéronomie du CNRS Jean-Yves Prado, CNES
First Assessments of EUVI Performance on STEREO SECCHI
Detectors of the New Projects at NAOC
Task Group Report: Ionosphere-Thermosphere
The Solar Dynamics Observatory:Waiting for a Launch Solar Cycle 24
esa. int/solar-orbiter/51168-summary/;
Space activities at Charles University
On the variations of the magnetospheric field line resonance frequency
Satellite mission ideas using EISCAT_3D
Transition Region and Coronal Explorer (TRACE)
CHEOPS - CHaracterizing ExOPlanet Satellite
NASA’s Global-scale Observations of the Limb and Disk (GOLD) Mission: Unprecedented Imaging of the Boundary Between Earth and Space Richard Eastes GOLD.
Presentation transcript:

Update of the French activities relevant to ILWS Jean-Yves Prado, CNES

Status of CNES projects PICARD Phase C/D in progress Launch planned for june 2009 Science Workshop at Yale in March, next in Toronto in July TARANIS Phase B will end in september NASA funding for JHU/APL XGRE inst through SMEX/MoO AO- No information Launch expected for 2011-12 SMESE Phase A ended in May ’08 Well attended Science Workshop in Paris last March Next step to be discussed during CNES ‘SPC’ this week – 4 options presented Launch objective 2012-2013 ALL BASED ON MYRIADE PLATEFORMES ILWS Prague, 11-12 June, 2008

PICARD SCIENTIFIC PRODUCTS in orbit: - Diameter, limb shape and asphericity in the continuum - TSI (x2) - 5 spectral channels (215,393, 535, 607, 782 nm) - Activity (images at 215 nm and Ca II)=> space weather - Solar oscillations from the ground : - diameter, limb shape and asphericity, - local atmosphere turbulence ILWS Prague, 11-12 June, 2008

THE PICARD SPACECRAFT SOVAP PREMOS2 SODISM ILWS Prague, 11-12 June, 2008

TARANIS OBJECTIVES Description - characterization of the sprites and associated emissions, measurements of their occurrence frequency and of their distribution at the scale of the earth. (caméras, EM waves, X and  spectra, high energy electrons) - study of the effects of the magnetic latitude and volcanic activity Implied mechanisms - determination of the nature of the triggering phenomena (cosmic radiation) - determination of the source mechanisms (EM waves, X and  spectra, high energy electrons) - study of the nature of the explosive dissipation of energy in the ionosphere and magnetosphere (EM waves, X and  spectra, high energy electrons) Global impact - determination of the effects on the upper atmosphere, ionosphere and magnetosphere (EM waves, high energy electrons, associated ground based measurements, other satellites) - evaluation of the coupling atmosphere -  ionosphere - magnetosphere and inter-planetary medium ILWS Prague, 11-12 June, 2008

Dedicated to understanding TARANIS Dedicated to understanding Atmosphere/ionosphere/magnetosphere coupling (sprites, elves, blue jets…) Microcameras + photometer -MCM- CEA (+JP) EM measurements -IEM- LPCE (+PL,TCH) X-gamma Detector -XGD- JHU/APL (USA), DNSC (DK) Detector of high Energy ElectronsCESR (+TCH) Quasi Sun Synchronous Orbit (2hrs LT drift/year) Phase B to end in September XGRE funding from NASA yet not known Launch >2011 ILWS Prague, 11-12 June, 2008

SMESE General View LYOT DESIR HEBS ILWS Prague, 11-12 June, 2008

SMESE payload required performances Wavelength/ Energy Field of View Spatial resolution Cadence LYOT : La imager 121.6 nm Full Disk 1.1 arcsec 10 s LYOT : La coronagraph 5*5 solar radii 2.3 arcsec 20 s DESIR : Infra-red Telescope 35 ≤ 1 ≤ 80 microns 100≤ 2 ≤ 250 microns 50 arcsec at 35 microns 100 ms HEBS 10-500keV 200keV-10MeV 10MeV-600MeV Full disk 1 s, down to 32 ms ILWS Prague, 11-12 June, 2008

SMESE Firsts First combined imaging (disk, corona) in Ly  with high time resolution and sensitivity to trace the development of CMEs in the low corona + first polarimetric corona measurements, First ever measurements of solar flares in the far infrared, key range for relativistic leptons and chromospheric plasma heated during flares, First hard X-ray/gamma ray spectrometry at the highest energies ever attained with a solar-dedicated instrument, to study the most energetic electrons and nuclear processes in the Sun’s atmosphere. Interest for Radiobiology ILWS Prague, 11-12 June, 2008

Mission sequence PICARD SMESE TARANIS ILWS Prague, 11-12 June, 2008

Others Operational coordination between DEMETER and C/NOFS STEREO Space Weather beacon Ground Station operational since Feb. Operational coordination between DEMETER and C/NOFS Radiation monitors onboard SAC-C, SAC-D, JASON 2 ILWS Prague, 11-12 June, 2008

ILWS Prague, 11-12 June, 2008

More than 20 spacecraft based on the same bus and systems MYRIADE SERIES More than 20 spacecraft based on the same bus and systems in flight or in preparation Bus waiting row 60x60x50 cm bus S-Band TTC (Kiruna/Toulouse) ILWS Prague, 11-12 June, 2008

MYRIADE CAPACITY Orbit inclination > 20° Altitude 600km< >1000km DNEPR launcher as the reference Geocentric, inertial, solar or along the velocity vector pointing Pointing precision of 0.1 ° (actuation), 5.10-3° (knowledge) Attitude control system in nominal mode uses a stellar sensor, four reaction wheels and three magnetic torquers up to 80 kg mass allocation to the P/L (when no propulsion/TM-X) Power available to the P/L > 60w (highly orbit dependant) Mass memory 16 Gbits S-Band 400 kb/s as baseline ILWS Prague, 11-12 June, 2008

MYRIADE OPTIONS propulsion DV ~80 m/s (DEMETER, TARANIS…) X-Band telemetry (>a few Gbits/day) TM rate 16-50 Mb/s depending on the ground station G/T additional sun pointing device (PICARD, LYOT/SMESE) quick deorbit kit under study ILWS Prague, 11-12 June, 2008

A few examples of the MYRIADE versatility DEMETER, TARANIS waves and particle instruments PARASOL Lidar for atmospheric science PICARD, SMESE Solar observation MICROSCOPE Fundamental physics ARGOS Localization ESSAIM, SPIRALE, ELINT Defense … commercial availability of the bus (ASTRIUM, AAS) DNEPR launch ARIANE 5 launch ILWS Prague, 11-12 June, 2008

FURTHER INTERNATIONAL COOPERATION Earth Observation as a paradigm? a unique object, many possible instruments curiosity driven science in competitition with monitoring science shift from mammoth s/c (ENVISAT…) to series of small specialized satellites A Solar Train? ILWS Prague, 11-12 June, 2008