Forecasting the space weather impact: the COMESEP Project

Publication: Research - peer-reviewJournal article – Annual report year: 2012

  • Author: Crosby, N. B.

    BIRA-IASB, Belgium

  • Author: Veronig, A.

    bUniversity of Graz, Austria

  • Author: Robbrecht, E.

    Royal Observatory of Belgium, Belgium

  • Author: Vennerstrøm, Susanne

    Solar System Physics, National Space Institute, Technical University of Denmark, Elektrovej, 2800, Kgs. Lyngby, Denmark

  • Author: Malandraki, O.

    National Observatory of Athens, Greece

  • Author: Dalla, S.

    University of Central Lancashire, United Kingdom

  • Author: Rodriguez, L.

    Royal Observatory of Belgium, Belgium

  • Author: Srivastava, N.

    Udaipur Solar Observatory, India

  • Author: Hesse, M.

    CCMC, NASA Goddard Space Flight Center, United States

  • Author: Odstrcil, D.

    George Mason University, United States

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The FP7 COronal Mass Ejections and Solar Energetic Particles (COMESEP) project is developing tools for forecasting geomagnetic storms and solar energetic particle (SEP) radiation storms. By analysis of historical data, complemented by the extensive data coverage of solar cycle 23, the key ingredients that lead to magnetic storm and SEP events and the factors that are responsible for false alarms are being identified. To enhance our understanding of the 3-D kinematics and interplanetary propagation of coronal mass ejections (CMEs), the structure, propagation and evolution of CMEs are being investigated. In parallel, the sources and propagation of SEPs are being examined and modelled. COMESEP is a unique cross-collaboration effort and bridges the gap between the SEP, CME and terrestrial effects scientific communities.
Original languageEnglish
JournalA I P Conference Proceedings Series
Publication date2012
Volume1500
Pages159-164
ISSN0094-243X
DOIs
StatePublished
CitationsWeb of Science® Times Cited: 0
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