Earth's Magnetosphere Model in the Framework of the IMPEx Data Model: Web-Services and Visualization Tools V. V. Kalegaev 1,, I. I. Alexeev 1, E. S. Belenkaya.

Slides:

Advertisements

Similar presentations

Kyoto Interop meeting, 17 May A VOTable application: Solar System objects in the VO J. Berthier 1, F. Vachier 1, V. Lainey 1, W. Thuillot 1, J.-E.

Advertisements

ICC 2009, Santiago de Chile Visualization of Glacier Surface Movement Samuel Wiesmann Institute of Cartography, ETH Zurich.

IWF Graz … 1 H. Lammer (1), M. L. Khodachenko (1), H. I. M. Lichtenegger (1), Yu. N. Kulikov (2), N. V. Erkaev (3), G. Wuchterl (4), P. Odert (5), M. Leitzinger.

1 Belov A., Baisultanova L., Eroshenko E., Yanke V. (IZMIRAN, Russia), Mavromichalaki H. (Athens University, Greece), Pchelkin V. (PGI, Russia) Magnetospheric.

Solar and Interplanetary Sources of Geomagnetic disturbances Yu.I. Yermolaev, N. S. Nikolaeva, I. G. Lodkina, and M. Yu. Yermolaev Space Research Institute.

PRECIPITATION OF HIGH-ENERGY PROTONS AND HYDROGEN ATOMS INTO THE UPPER ATMOSPHERES OF MARS AND VENUS Valery I. Shematovich Institute of Astronomy, Russian.

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.

Solar and STP Physics with AstroGrid 1. Mullard Space Science Laboratory, University College London. 2. School of Physics and Astronomy, University of.

1 Grades 3 - 5: Introduction. 2 Better Observation Of The Sun And Earth Importance of Space Technology.

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

Finding Useful Information ON THE WEB. Published papers Most published papers in astronomy can be found on the NASA Astrophysics Data System: Most published.

Space Physics at Mars Paul Withers Journal Club Research Talk Center for Space Physics, Boston University Aims: Show students how principles.

NASA World Wind. What is NASA World Wind? A richly interactive 3D planetary visualization tool. Smart client architecture. Portal for NASA data. Integrates.

Distributed Data Analysis & Dissemination System (D-DADS) Prepared by Stefan Falke Rudolf Husar Bret Schichtel June 2000.

UTILIZING SPENVIS FOR EARTH ORBIT ENVIRONMENTS ASSESSMENTS: RADIATION EXPOSURES, SEE, and SPACECRAFT CHARGING Brandon Reddell and Bill Atwell THE BOEING.

Lessons learned from CCMC-led community-wide Model Validation Challenges. Outlook on international coordination of M&V activities. MODELS  DATA  TOOLS.

PLANETOCOSMICS L. Desorgher, M. Gurtner, E.O. Flückiger, and P. Nieminen Physikalisches Institut, University of Bern ESA/ESTEC.

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

Atmosphere - Ionosphere - Magnetosphere Working Group Paul Kintner Nicky Fox Mary Hudson Janet Kozyra Michelle Thompson George Siscoe Dave Byers Howard.

Name Here 75 pts. Zoom in and explore the solar system for 5-7 minutes… write down 5 observations from this animation… pts Use these.

Academician Sergey Vernov November, Joe Allen: According to Herb Sauer, a PhD candidate at the University of Iowa at this time, he was the first.

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

Y. Bouderba, S. Naitamor, O. Boumia Research Center on Astronomy, Astrophysics and Geophysics. CRAAG (Algeria). 1 International School of Space Science,

AMDA and CLweb Two complementary web-based services for spacecraft data exploitation with help from LESIA and support from CNES and CNRS Benoit Lavraud,

Computer Simulations in Solar System Physics Mats Holmström Swedish Institute of Space Physics (IRF) Forskarskolan i rymdteknik Göteborg 12 September 2005.

Comparative Aurora Cross-body –Intrinsic magnetospheres (e.g., Earth, Giant planets) –Induced magnetospheres (e.g., Venus, Mars, Titan) Cross-wavelength:

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

JAXA’s Space Exploration Scenario for the Next Twenty Years - Science Strategy - Masato Nakamura Steering Committee of Space Science Institute of Space.

AMDA, Automated Multi-Dataset Analysis: A web-based service provided by the CDPP. Jacquey 1 C., V. Génot 1, E. Budnik 2, R. Hitier 3, M. Bouchemit 1, M.

International Conference on Comparative Planetology: Venus - Earth - Mars ESTEC, Noordwijk, The Netherlands, Thursday 14 May :10:00, Abstract #

Space Research Institute Graz Austrian Academy of Sciences CERN, Geneve, June 2006 Helmut O. Rucker Exploring the Planets and Moons in our Solar System.

Computational Model of Energetic Particle Fluxes in the Magnetosphere Computer Systems Yu (Evans) Xiang Mentor: Dr. John Guillory, George Mason.

The PLANETOCOSMICS Geant4 application L. Desorgher Physikalisches Institut, University of Bern.

Nowcast model of low energy electrons (1-150 keV) for surface charging hazards Natalia Ganushkina Finnish Meteorological Institute, Helsinki, Finland.

Solar Wind and Coronal Mass Ejections

Space Weather Modelling: from Science to Applications Chair: M. Dinguirard ONERA.

Currently the Solar Energetic Particle Environment Models (SEPEM) system treats only protons within the interplanetary environment, and the shielding analysis.

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.,

Exploring Jupiter with Radio Waves W. S. Kurth The University of Iowa Iowa City, IA.

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.

SolarFlows Dr. Gabriele Pierantoni (TCD). Contents What is Heliophysics ? How could workflows help ? Some examples What we are doing...

ASTRONOMY 8850: Planetary Sciences Why Sciences?.

Plasma Node demonstrators 1/Registry : –Set of XML descriptors of planetary plasma data (MAPSKP, VEX, MEX ) –Compliant with the SPASE data model

Distributed Data Analysis & Dissemination System (D-DADS ) Special Interest Group on Data Integration June 2000.

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

MERCURY VENSUS MARS JUPITER SATURN URANUS.

Introduction to ESA science classroom activities Rebecca Barnes HE Space operations for ESA 11/07/2011.

AHM04: Sep 2004 Nottingham CCLRC e-Science Centre eMinerals: Environment from the Molecular Level Managing simulation data Lisa Blanshard e- Science Data.

RPWI Team Meeting, Sep. 2010, Roma Magnetic Loop Antenna (MLA) Scientific Objectives A. Marchaudon, V. Krasnoselskikh, T. Dudok de Wit, C. Cavoit,

29 ICRC, Pune, India, 2005 Geomagnetic effects on cosmic rays during the very strong magnetic storms in November 2003 and November 2004 Belov (a), L. Baisultanova.

Solar Wind Propagation Tool Chihiro Tao 1,2, Nicolas Andre 1, Vincent Génot 1, Alexis P. Rouillard 1, Elena Budnik 1, Arnaud Biegun 1, Andrei Fedorov 1.

OVT status Yuri Khotyaintsev Swedish Institute of Space Physics, Uppsala and the OVT team ovt.irfu.se November 18, 2015.

Magnetic Fields. Magnetic Field of a bar magnet I. Field of a bar magnet The forces of repulsion and attraction in bar magnets are due to the magnetic.

Topic 7: The Solar System Close Up

Comparisons between Magnetic field Perturbations and model dipole moments at Europa Derek Podowitz EAS /28/2011.

ICESTAR: Solar-terrestrial and aeronomy research during the International Polar Year Kirsti Kauristie1, Allan Weatherwax2, Richard Harrison3, Richard.

V. M. Lipunov, E. S. Gorbovskoy

The IMPEx Data Model and Protocol

The Sun: Portrait of a G2V star

Topic 7: The Solar System Close Up

Physics-based simulation for visual computing applications

Meeting on Solar Wind Turbulence, Kennebunkport, June 4-7, 2013

Computational Model of Energetic Particle Fluxes in the Magnetosphere

Quantification of solar wind parameters from measurments by SOHO and DSCOVR spacecrafts during series of Interplanetary Coronal Mass Ejections in the.

Grades 3 - 5: Introduction

The Planets of our Solar System The Terrestrial Planets

Grades 3 - 5: Introduction

Maria Teresa Capria December 15, 2009 Paris – VOPlaneto 2009

Getting Planetary Science Data

Presentation transcript:

Earth's Magnetosphere Model in the Framework of the IMPEx Data Model: Web-Services and Visualization Tools V. V. Kalegaev 1,, I. I. Alexeev 1, E. S. Belenkaya 1, L.R. Mukhametdinova 1, M. L. Khodachenko 2,1, V. Génot 3, E. J. Kallio 4, T. Al-Ubaidi 3, R. Modolo 5 1 Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University (SINP MSU), Moscow, Russian Federation 2 Space Research Institute, Austrian Academy of Science, Graz, Austria 3 IRAP, CNRS, Toulouse, France 4 Finnish Meteorological Institute, Helsinki, Finland 5 LATMOS, CNRS/Université de Versailles Saint-Quentin, Guyancourt, France

Data providers IMPEx project - Integrated Medium for Planetary Exploration Observational data Simulation models SINP PMM SINP PMM HMM … … Spacecraft measurements Spacecraft measurements IMPEx User User Layer Tools Layer Resource Layer In browser clientsJava client CLWebAMDA3DView can be more Virtual workspace impexconf.xml AMDA Server CLWeb Server 3DView Server Precalculated data access HMM/PMM Environment PMM/HMM Simulation Archives HMM/PMM Computational Services Compute Services SOAP methods.wsdl tree.xml IMPEx portal

Paraboloid model Paraboloid model of the Earth's magnetosphere has been developed at Moscow State University to represent correctly the electrodynamics processes in the near-Earth's space. This model is intended to calculate the magnetic field generated by a variety of current systems located on the boundaries and within the boundaries of the Earth's magnetosphere under a wide range of environmental conditions, quiet and disturbed, affected by Solar-Terrestrial interactions simulated by Solar activity such as Solar Flares and related phenomena which induce terrestrial magnetic disturbances such as Magnetic Storms. The model depends on a small set of physical input parameters, which characterize the intensity of large-scale magnetospheric current systems and their location. PMM structure BM = B1+B2 B2 = Bsd( , R1) + Bt( , R1,R2,  )+ Br( ,br) + Bsr( ,R1,br) + Bfac(I||) B = + … + + Bfac Bcfl Btail

Common set of web-services between simulation databases and tools Interpolation in the precalculated cubes: points lines cuts Interpolation in the precalculated cubes: points lines cuts Calculation of the magnetic field: Earth: in points, in different time moments; in points in one time moment; field lines from selected points; along spacecraft trajectories; in a selected cube; Mercury, Saturn, Jupiter: in points, in different time moment; in a selected cube; Calculation of the magnetic field: Earth: in points, in different time moments; in points in one time moment; field lines from selected points; along spacecraft trajectories; in a selected cube; Mercury, Saturn, Jupiter: in points, in different time moment; in a selected cube;

Input parameters can be taken from OMNI by date, or inserted manually