This article has an erratum: [https://doi.org/10.1051/swsc/2016040]
J. Space Weather Space Clim.
Volume 5, 2015
Satellite mission concepts developed at the Alpbach 2013 Summer School on space weather
|Number of page(s)||14|
|Published online||17 February 2015|
A Space Weather mission concept: Observatories of the Solar Corona and Active Regions (OSCAR)
Département de Physique, Université de Montréal, C.P. 6128
Succ. Centre-Ville, Montréal, QC, H3C-3J7, Canada
2 Laboratoire AIM Paris-Saclay, CEA/Irfu Université Paris-Diderot CNRS/INSU, 91191 Gif-sur-Yvette, France
3 Institute of Experimental and Applied Physics, University of Kiel, Kiel, Germany
4 Mullard Space Science Laboratory, University College London, Dorking, United Kingdom
5 Institut für Astrophysik, University of Vienna, Vienna, Austria
6 FOTEC – Department of Aerospace Engineering, Wiener Neustadt, Austria
7 Finnish Meteorological Institute, Helsinki, Finland
8 Department of Physics, University of Helsinki, Helsinki, Finland
9 Royal Observatory of Belgium, Brussels, Belgium
10 German Aerospace Centre (DLR), Institute of Aerospace Medicine, Cologne, Germany
11 Institut Supérieur de l’Aéronautique et de l’Espace, Toulouse, France
12 La Sapienza – University of Rome, Italy
13 Department of Physics, Free University of Berlin, Berlin, Germany
14 Danish Space Research Institute, Copenhagen, Denmark
15 School of Medicine and Medical Sciences, University College Dublin, Dublin, Ireland
16 Dpto. de Astrofísica y CC. de la Atmósfera, Universidad Complutense de Madrid, 28040 Madrid, Spain
17 Department of Physics, University of Oslo, Norway
18 ESA/ESTEC, Noordwijk, The Netherlands
19 Space Research Institute, Austrian Academy of Sciences, Austria
* Corresponding author: firstname.lastname@example.org
Accepted: 1 September 2014
Coronal Mass Ejections (CMEs) and Corotating Interaction Regions (CIRs) are major sources of magnetic storms on Earth and are therefore considered to be the most dangerous space weather events. The Observatories of Solar Corona and Active Regions (OSCAR) mission is designed to identify the 3D structure of coronal loops and to study the trigger mechanisms of CMEs in solar Active Regions (ARs) as well as their evolution and propagation processes in the inner heliosphere. It also aims to provide monitoring and forecasting of geo-effective CMEs and CIRs. OSCAR would contribute to significant advancements in the field of solar physics, improvements of the current CME prediction models, and provide data for reliable space weather forecasting. These objectives are achieved by utilising two spacecraft with identical instrumentation, located at a heliocentric orbital distance of 1 AU from the Sun. The spacecraft will be separated by an angle of 68° to provide optimum stereoscopic view of the solar corona. We study the feasibility of such a mission and propose a preliminary design for OSCAR.
Key words: Missions / Corona / Active region / Interplanetary Coronal Mass Ejection (CME) / Corotating Interaction Regions (CIR)
© A. Strugarek et al., Published by EDP Sciences 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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