Observation of shocks associated with CMEs in 2007

The interaction of CMEs with the solar wind can lead to the formation of interplanetary shocks. Ions accelerated at these shocks contribute to the solar energetic protons observed in the vicinity of the Earth. Recently a joint analysis of Venus Express (VEX) and STEREO data by Russell et al. (20...

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Main Authors: H. Aryan, M. A. Balikhin, A. Taktakishvili, T. L. Zhang
Format: Article
Language:English
Published: Copernicus Publications 2014-03-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/32/223/2014/angeo-32-223-2014.pdf
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author H. Aryan
M. A. Balikhin
A. Taktakishvili
T. L. Zhang
author_facet H. Aryan
M. A. Balikhin
A. Taktakishvili
T. L. Zhang
author_sort H. Aryan
collection DOAJ
description The interaction of CMEs with the solar wind can lead to the formation of interplanetary shocks. Ions accelerated at these shocks contribute to the solar energetic protons observed in the vicinity of the Earth. Recently a joint analysis of Venus Express (VEX) and STEREO data by Russell et al. (2009) have shown that the formation of strong shocks associated with Co-rotating Interaction Regions (CIRs) takes place between the orbits of Venus and the Earth as a result of coalescence of weaker shocks formed earlier. The present study uses VEX and Advanced Composition Explorer (ACE) data in order to analyse shocks associated with CMEs that erupted on 29 and 30 July 2007 during the solar wind conjunction period between Venus and the Earth. For these particular cases it is shown that the above scenario of shock formation proposed for CIRs also takes place for CMEs. Contradiction with shock formation resulting from MHD modelling is explained by inability of classical MHD to account for the role of wave dispersion in the formation of the shock.
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spelling doaj.art-f25e9696235c416aa21670c982ce89a02022-12-22T00:18:38ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762014-03-013222323010.5194/angeo-32-223-2014Observation of shocks associated with CMEs in 2007H. Aryan0M. A. Balikhin1A. Taktakishvili2T. L. Zhang3Department of Automatic Control and Systems Engineering, University of Sheffield, Sheffield, UKDepartment of Automatic Control and Systems Engineering, University of Sheffield, Sheffield, UKNASA Goddard Space Flight Center, Greenbelt, Maryland, USASpace Research Institute, Austrian Academy of Sciences, Graz, AustriaThe interaction of CMEs with the solar wind can lead to the formation of interplanetary shocks. Ions accelerated at these shocks contribute to the solar energetic protons observed in the vicinity of the Earth. Recently a joint analysis of Venus Express (VEX) and STEREO data by Russell et al. (2009) have shown that the formation of strong shocks associated with Co-rotating Interaction Regions (CIRs) takes place between the orbits of Venus and the Earth as a result of coalescence of weaker shocks formed earlier. The present study uses VEX and Advanced Composition Explorer (ACE) data in order to analyse shocks associated with CMEs that erupted on 29 and 30 July 2007 during the solar wind conjunction period between Venus and the Earth. For these particular cases it is shown that the above scenario of shock formation proposed for CIRs also takes place for CMEs. Contradiction with shock formation resulting from MHD modelling is explained by inability of classical MHD to account for the role of wave dispersion in the formation of the shock.https://www.ann-geophys.net/32/223/2014/angeo-32-223-2014.pdf
spellingShingle H. Aryan
M. A. Balikhin
A. Taktakishvili
T. L. Zhang
Observation of shocks associated with CMEs in 2007
Annales Geophysicae
title Observation of shocks associated with CMEs in 2007
title_full Observation of shocks associated with CMEs in 2007
title_fullStr Observation of shocks associated with CMEs in 2007
title_full_unstemmed Observation of shocks associated with CMEs in 2007
title_short Observation of shocks associated with CMEs in 2007
title_sort observation of shocks associated with cmes in 2007
url https://www.ann-geophys.net/32/223/2014/angeo-32-223-2014.pdf
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