Forecasting the space weather impact: the COMESEP Project

N. B. Crosby; A. Veronig; E. Robbrecht; Susanne Vennerstrøm; O. Malandraki; S. Dalla; L. Rodriguez; N. Srivastava; M. Hesse; D. Odstrcil

doi:10.1063/1.4768760

Forecasting the space weather impact: the COMESEP Project

N. B. Crosby
, A. Veronig
, E. Robbrecht
, Susanne Vennerstrøm
, O. Malandraki
, S. Dalla
, L. Rodriguez
, N. Srivastava
, M. Hesse
, D. Odstrcil

Royal Belgian Institute for Space Aeronomy
University of Graz
Royal Observatory of Belgium
National Observatory of Athens
University of Central Lancashire
Udaipur Solar Observatory
NASA Goddard Space Flight Center
George Mason University

Research output: Contribution to journal › Journal article › Research › peer-review

Abstract

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 language	English
Journal	A I P Conference Proceedings Series
Volume	1500
Pages (from-to)	159-164
ISSN	0094-243X
DOIs	https://doi.org/10.1063/1.4768760
Publication status	Published - 2012

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title = "Forecasting the space weather impact: the COMESEP Project",

abstract = "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.",

author = "Crosby, \{N. B.\} and A. Veronig and E. Robbrecht and Susanne Vennerstr{\o}m and O. Malandraki and S. Dalla and L. Rodriguez and N. Srivastava and M. Hesse and D. Odstrcil",

year = "2012",

doi = "10.1063/1.4768760",

language = "English",

volume = "1500",

pages = "159--164",

journal = "A I P Conference Proceedings Series",

issn = "0094-243X",

publisher = "American Institute of Physics",

}

TY - JOUR

T1 - Forecasting the space weather impact

T2 - the COMESEP Project

AU - Crosby, N. B.

AU - Veronig, A.

AU - Robbrecht, E.

AU - Vennerstrøm, Susanne

AU - Malandraki, O.

AU - Dalla, S.

AU - Rodriguez, L.

AU - Srivastava, N.

AU - Hesse, M.

AU - Odstrcil, D.

PY - 2012

Y1 - 2012

N2 - 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.

AB - 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.

U2 - 10.1063/1.4768760

DO - 10.1063/1.4768760

M3 - Journal article

SN - 0094-243X

VL - 1500

SP - 159

EP - 164

JO - A I P Conference Proceedings Series

JF - A I P Conference Proceedings Series

ER -

Forecasting the space weather impact: the COMESEP Project

Abstract

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