Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1
The Double Star TC-1 magnetosheath pass on 26 February 2004 is used to investigate magnetic field fluctuations. Strong compressional signatures which last for more than an hour have been found near the magnetopause behind a quasi-perpendicular bow shock. These compressional structures are most l...
Main Authors: | , , , , |
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Format: | Article |
Language: | English |
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Copernicus Publications
2009-01-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/27/351/2009/angeo-27-351-2009.pdf |
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author | J. Du C. Wang T. L. Zhang M. Volwerk C. Carr |
author_facet | J. Du C. Wang T. L. Zhang M. Volwerk C. Carr |
author_sort | J. Du |
collection | DOAJ |
description | The Double Star TC-1 magnetosheath pass on 26 February 2004 is used
to investigate magnetic field fluctuations. Strong compressional
signatures which last for more than an hour have been found near the
magnetopause behind a quasi-perpendicular bow shock. These
compressional structures are most likely mirror mode waves. There is
a clear wave transition in the magnetosheath which probably results
from the change of the interplanetary magnetic field (IMF) cone
angle. The wave characteristics in the magnetosheath are strongly
controlled by the type of the upstream bow shock. |
first_indexed | 2024-12-10T15:14:09Z |
format | Article |
id | doaj.art-570463d4c78e43c4945d9f90bffd3f48 |
institution | Directory Open Access Journal |
issn | 0992-7689 1432-0576 |
language | English |
last_indexed | 2024-12-10T15:14:09Z |
publishDate | 2009-01-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Annales Geophysicae |
spelling | doaj.art-570463d4c78e43c4945d9f90bffd3f482022-12-22T01:43:50ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762009-01-012735135510.5194/angeo-27-351-2009Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1J. Du0C. Wang1T. L. Zhang2M. Volwerk3C. Carr4State Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, ChinaState Key Laboratory of Space Weather, Center for Space Science and Applied Research, Chinese Academy of Sciences, Beijing, ChinaSpace Research Institute, Austrian Academy of Sciences, 8042 Graz, AustriaSpace Research Institute, Austrian Academy of Sciences, 8042 Graz, AustriaThe Blackett Laboratory, Imperial College, London, UKThe Double Star TC-1 magnetosheath pass on 26 February 2004 is used to investigate magnetic field fluctuations. Strong compressional signatures which last for more than an hour have been found near the magnetopause behind a quasi-perpendicular bow shock. These compressional structures are most likely mirror mode waves. There is a clear wave transition in the magnetosheath which probably results from the change of the interplanetary magnetic field (IMF) cone angle. The wave characteristics in the magnetosheath are strongly controlled by the type of the upstream bow shock.https://www.ann-geophys.net/27/351/2009/angeo-27-351-2009.pdf |
spellingShingle | J. Du C. Wang T. L. Zhang M. Volwerk C. Carr Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1 Annales Geophysicae |
title | Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1 |
title_full | Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1 |
title_fullStr | Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1 |
title_full_unstemmed | Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1 |
title_short | Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1 |
title_sort | mirror waves and mode transition observed in the magnetosheath by double star tc 1 |
url | https://www.ann-geophys.net/27/351/2009/angeo-27-351-2009.pdf |
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