Mexico-Russia nanosatellite for earthquakes precursors monitoring Pulinets S. 1, Landeros S. 2, Bisiacchi G. 3, García-Garduño V. 2, García J.-L. 2, De.

Slides:



Advertisements
Similar presentations
Wave-particles interaction in radiation belt region Hanna Rothkaehl Space Research Center, PAS Bartycka 18 A Warsaw, Poland,
Advertisements

Sergey Pulinets 1,2 1 Space Research Institute, RAS 2 Fiodorov Institute of Applied Geophysics, Roshydromet Russia.
Global Positioning System. What is GPS? A worldwide radio-navigation system – constellation of 24 satellites –with 5 ground stations GPS uses these “man-made.
Workshop „X-ray Spectroscopy and Plasma Diagnostics from the RESIK, RHESSI and SPIRIT Instruments”, 6 – 8 December 2005, Wrocław Spectroscopy Department.
Cosmic Ray Using for Monitoring and Forecasting Dangerous Solar Flare Events Lev I. Dorman (1, 2) 1. Israel Cosmic Ray & Space Weather Center and Emilio.
J C Foster MIT Haystack Observatory Yosemite 2002 Plasma Tails & Ionospheric SED.
Plasmas in Space: From the Surface of the Sun to the Orbit of the Earth Steven R. Spangler, University of Iowa Division of Plasma Physics, American Physical.
Further development of modeling of spatial distribution of energetic electron fluxes near Europa M. V. Podzolko 1, I. V. Getselev 1, Yu. I. Gubar 1, I.
A student satellite initiative Indian Institute of Technology Madras.
The DEMETER satellite: Payload, Operations and Data
From Geo- to Heliophysical Year: Results of CORONAS-F Space Mission International Conference «50 Years of International Geophysical Year and Electronic.
Magnetospheric Morphology Prepared by Prajwal Kulkarni and Naoshin Haque Stanford University, Stanford, CA IHY Workshop on Advancing VLF through the Global.
1 K. Stasiewicz, Plasma Space Science Center, NCKU Swedish Institute of Space Physics, Uppsala Multi-spacecraft studies of nonlinear waves.
Earthquake: 05:46:23 UT Tohoku Tsunami Seen in Ionosphere Using GPS Compared with JPL’s Song Tsunami Model Attila Komjathy (335G), David Galvan (335G),
Radio Waves Diagnostics of Ionospheric Plasma 1Space Research Center, Polish Academy of Sciences, Warsaw, Poland 2 Swedish Institute of Space Physics,
Centre de Toulouse Radiation interaction with matter 1.
Accuracy assessment of the space weather characteristics forecasts used in the Russian Federal Space Agency Monitoring System V. Anashin 1, G. Protopopov.
Interrelation between Cosmic Rays, Magnetosphere particles and the Earth Atmospheric Phenomena- Prospects of Experimental Study from Satellites M.I. Panasyuk.
RELEC project (Relativistic ELECtrons). Unified platform “Karat” for small spacecraft 2 MICROSATELLITE KARAT FOR PLANETARY MISSIONS, ASTROPHYSICAL AND.
Ionosphere Precursors to the Dec 30, 2010 Mexicali Earthquake Rachel Thessin, CSI 763, May 11, 2010.
THE STUDY OF ELECTROMAGNETIC PARAMETERS OF SPACE WEATHER Thunderstorms and Elementary Particle Acceleration (TEPA-2010) MICRO-SATELLITE “CHIBIS- M”
ILWS and Finland Hannu Koskinen Finland and ILWS2 ILWS science in Finland Finnish Meteorological Institute, Helsinki Magnetospheres.
RUSSIAN SPACE MISSIONS FOR SOLAR-TERRESTRIAL SCIENCE ILWS-2011 A.A. Petrukovich, L.M. Zelenyi Space Research Institute V.D. Kuznetsov IZMIRAN.
Multilayer thin film technology for the STS electronic high density interconnection E. Atkin Moscow Engineering Physics Institute (State University) –
NOSCI Infrastructure for Lunar Observatories Bremen, Germany March 22 – 24, 2005 NanOspace-1 SCientific Instruments Jan Bergman Swedish Institute of Space.
RELEC project (Relativistic ELECtrons). Satellites Low altitudes Geostationary Balloons Arctic Antarctic Ionosphere Atmosphere particles Space and balloon.
Your Name Your Title Your Organization (Line #1) Your Organization (Line #2) About technique of alignment and stacking of TGF Vybornov V. Pozanenko.
Space fluorescence detectors TUS/KLYPVE for study of UHECR. (Italian-Russian seminar on space detectors) 19 October 2005 B. A. KHRENOV 19 October 2005.
Graz, June 2007 The DEMETER mission: Objectives and first results M. Parrot LPCE/CNRS 3A, Avenue de la Recherche Orléans cedex 2, France
A.V. Belov 1, E. A. Eroshenko 1, H. Mavromichalaki 2, V.A. Oleneva 1, A. Papaioannou 2, G. Mariatos 2, V. G. Yanke 1 (1) Institute of Terrestrial Magnetism,
G.K. Garipov 1, B.A. Khrenov 1, P.A. Klimov 1, V.S. Morozenko 1, M.I. Panasyuk 1, V.I. Tulupov 1, V.M. Shahparonov 1, S.A. Sharakin 1, S.I. Svertilov 1,
Joint International GRACE Science Team Meeting and DFG SPP 1257 Symposium, Oct. 2007, GFZ Potsdam Folie 1 Retrieval of electron density profiles.
Geo-Space observation of atmospheric environmental effects associated with 2011 Fukushima nuclear accident Our approach of using multiple geo-space observation.
1 IGY The ALERT signal of ground level enhancements of solar cosmic rays: physics basis, the ways of realization and development Anashin V., Belov A.,
Programa de Satélites Científicos e Experimentos do INPE MCE Equatorial Atmosphere Research Satellite Monitor e Imageador de Raios-X Missão Clima Espacial.
Exploitation of Space Ionizing Radiation Monitoring System in Russian Federal Space Agency STRUCTURE OF THE MONITORING SYSTEM The Monitoring System includes.
Earth’s Magnetosphere NASA Goddard Space Flight Center
The spatial and temporal distribution of solar and galactic cosmic rays S. V. Tasenko 1, P. V. Shatov 1, I. A. Skorokhodov 1, I. V. Getselev 1,2, M. Podzolko.
UV And Red-IR Radiation Flashes Energy Characteristics Measured by UV&IR Detector On-Board “Universitetsky-Tatiana-2” Satellite. G.K. Garipov 1, B.A. Khrenov.
Topics in Space Weather Earth Atmosphere & Ionosphere
Dark Matter Search Using High Resolution Emulsion M. University.
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.
NASA 2001 Mars Odyssey page 1 Workshop HEND Russian Aviation and Space Agency Institute for Space Research Present knowledge of HEND efficiency.
Radiation Storms in the Near Space Environment Mikhail Panasyuk, Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University.
Contact Information: Dr. Howard J. Singer, Chief Research and Development Division NOAA Space Environment Center 325 Broadway Boulder, CO
Space Weather in Earth’s magnetosphere MODELS  DATA  TOOLS  SYSTEMS  SERVICES  INNOVATIVE SOLUTIONS Space Weather Researc h Center Masha Kuznetsova.
Predicting Ionospheric Densities and Scintillation with the Communication / Navigation Outage Forecasting System (C/NOFS) Mission Chin S. Lin 1, O. de.
The SPHERE Project Antarctic Balloon-Borne Measurements Of Cosmic Rays Spectrum In Energy Range 1-100EeV Rem Antonov – Moscow State University R.A. Antonov,
European Space Agency, version 1.0, Coordination Group for Meteorological Satellites - CGMS ESA SSA Programme Plans for Space Weather Missions.
High Energy Observational Astrophysics. 1 Processes that emit X-rays and Gamma rays.
Earth’s Magnetosphere Space Weather Training Kennedy Space Center Space Weather Research Center.
KMA Space Weather Service Presented to CGMS-44 on Working Group SWTT.
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.
AGILE as particle monitor: an update
Xenon gamma-ray detector for “SIGNAL” experiment
JMA Report on Satellite-based Space Weather Activities in Japan
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.
A Relation between Solar Flare Manifestations and the GLE Onset
V. M. Lipunov, E. S. Gorbovskoy
Carbon-Foil for reducing first strike issues
RESTORATION OF THE MARSIS SIGNAL FOR SUBSURFACE SOUNDING
Accommodation From DoI studies
Study of 20 January 2005 solar flare area by certain gamma-ray lines
Meeting on Solar Wind Turbulence, Kennebunkport, June 4-7, 2013
Ionospheric Scintilatiton and TEC maps
Accommodation From DoI studies
Task Group Report: Ionosphere-Thermosphere
Satellite mission ideas using EISCAT_3D
Presentation transcript:

Mexico-Russia nanosatellite for earthquakes precursors monitoring Pulinets S. 1, Landeros S. 2, Bisiacchi G. 3, García-Garduño V. 2, García J.-L. 2, De la Rosa S. 2, Brekhov O. 4, Panasyuk M. 5, Grigoryan O. 5, Selivanov 6, Bergman J. 7 1 Institute of Geophysics, UNAM, Mexico 1 3 Ingeneering Faculty, UNAM, Mexico 3 Techological Center “Aragon”, UNAM, Mexico 4 Moscow Aviation Institute, Russia 5 Skobeltsyn Institute of Nuclear Physics, Moscow State University, Russia 6 RNII KP, Russia, 7 Swedish Institute of Space Physics, Sweden

Nanosatellite platform TNS-1 Circular platform of 500 mm diameter (aluminium – carbon plastic) Side А – solar panels Side B – payload Passive and active orientation Absence of the moving components Passive thermoregulation

Payload structure of the TNS-1

Payload selection  Price  Ability to register precursors  Accommodation to platform  Possibility to use in educational purposes

March 22, 2005 (Sumatra-2)

Ion density map 22 of March

Coronas

Effects in equatorial anomaly Pulinets and Legen’ka, 2002

Wave image of the ionosphere

Energetic particles

Swedish nanosatellite

UNAMSAT-3 Langmuir probevariations of the electron density and temperature Particle detectors110 keV - 80 MeV HF radiospectrometer 0.1 – 15 MHz GPS receiver

Ground support

Rector of UNAM, Huan Ramón de la Fuente in Moscow