Influences on the radius of the auroral oval

We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interv...
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Autor*in:	S. E. Milan [verfasserIn] J. Hutchinson [verfasserIn] P. D. Boakes [verfasserIn] B. Hubert [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2009

Übergeordnetes Werk:	In: Annales Geophysicae - Copernicus Publications, 2002, 27(2009), Seite 2913-2924
Übergeordnetes Werk:	volume:27 ; year:2009 ; pages:2913-2924

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc Journal toc

DOI / URN:	10.5194/angeo-27-2913-2009

Katalog-ID:	DOAJ016492277

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520			\|a We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current.
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spelling	10.5194/angeo-27-2913-2009 doi (DE-627)DOAJ016492277 (DE-599)DOAJ0d8ffaaac15c4ba1bfed78b4a76567f3 DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Influences on the radius of the auroral oval 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current. Science Q Physics Geophysics. Cosmic physics J. Hutchinson verfasserin aut P. D. Boakes verfasserin aut P. D. Boakes verfasserin aut B. Hubert verfasserin aut In Annales Geophysicae Copernicus Publications, 2002 27(2009), Seite 2913-2924 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:27 year:2009 pages:2913-2924 https://doi.org/10.5194/angeo-27-2913-2009 kostenfrei https://doaj.org/article/0d8ffaaac15c4ba1bfed78b4a76567f3 kostenfrei https://www.ann-geophys.net/27/2913/2009/angeo-27-2913-2009.pdf kostenfrei https://doaj.org/toc/0992-7689 Journal toc kostenfrei https://doaj.org/toc/1432-0576 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2014 GBV_ILN_2048 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 27 2009 2913-2924
allfields_unstemmed	10.5194/angeo-27-2913-2009 doi (DE-627)DOAJ016492277 (DE-599)DOAJ0d8ffaaac15c4ba1bfed78b4a76567f3 DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Influences on the radius of the auroral oval 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current. Science Q Physics Geophysics. Cosmic physics J. Hutchinson verfasserin aut P. D. Boakes verfasserin aut P. D. Boakes verfasserin aut B. Hubert verfasserin aut In Annales Geophysicae Copernicus Publications, 2002 27(2009), Seite 2913-2924 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:27 year:2009 pages:2913-2924 https://doi.org/10.5194/angeo-27-2913-2009 kostenfrei https://doaj.org/article/0d8ffaaac15c4ba1bfed78b4a76567f3 kostenfrei https://www.ann-geophys.net/27/2913/2009/angeo-27-2913-2009.pdf kostenfrei https://doaj.org/toc/0992-7689 Journal toc kostenfrei https://doaj.org/toc/1432-0576 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2014 GBV_ILN_2048 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 27 2009 2913-2924
allfieldsGer	10.5194/angeo-27-2913-2009 doi (DE-627)DOAJ016492277 (DE-599)DOAJ0d8ffaaac15c4ba1bfed78b4a76567f3 DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Influences on the radius of the auroral oval 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current. Science Q Physics Geophysics. Cosmic physics J. Hutchinson verfasserin aut P. D. Boakes verfasserin aut P. D. Boakes verfasserin aut B. Hubert verfasserin aut In Annales Geophysicae Copernicus Publications, 2002 27(2009), Seite 2913-2924 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:27 year:2009 pages:2913-2924 https://doi.org/10.5194/angeo-27-2913-2009 kostenfrei https://doaj.org/article/0d8ffaaac15c4ba1bfed78b4a76567f3 kostenfrei https://www.ann-geophys.net/27/2913/2009/angeo-27-2913-2009.pdf kostenfrei https://doaj.org/toc/0992-7689 Journal toc kostenfrei https://doaj.org/toc/1432-0576 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2014 GBV_ILN_2048 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 27 2009 2913-2924
allfieldsSound	10.5194/angeo-27-2913-2009 doi (DE-627)DOAJ016492277 (DE-599)DOAJ0d8ffaaac15c4ba1bfed78b4a76567f3 DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Influences on the radius of the auroral oval 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current. Science Q Physics Geophysics. Cosmic physics J. Hutchinson verfasserin aut P. D. Boakes verfasserin aut P. D. Boakes verfasserin aut B. Hubert verfasserin aut In Annales Geophysicae Copernicus Publications, 2002 27(2009), Seite 2913-2924 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:27 year:2009 pages:2913-2924 https://doi.org/10.5194/angeo-27-2913-2009 kostenfrei https://doaj.org/article/0d8ffaaac15c4ba1bfed78b4a76567f3 kostenfrei https://www.ann-geophys.net/27/2913/2009/angeo-27-2913-2009.pdf kostenfrei https://doaj.org/toc/0992-7689 Journal toc kostenfrei https://doaj.org/toc/1432-0576 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ SSG-OLC-PHA GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_267 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_2003 GBV_ILN_2014 GBV_ILN_2048 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 27 2009 2913-2924
language	English
source	In Annales Geophysicae 27(2009), Seite 2913-2924 volume:27 year:2009 pages:2913-2924
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callnumber-first	Q - Science
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topic_title	QC1-999 QC801-809 Influences on the radius of the auroral oval
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title	Influences on the radius of the auroral oval
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title_sort	influences on the radius of the auroral oval
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title_auth	Influences on the radius of the auroral oval
abstract	We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current.
abstractGer	We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current.
abstract_unstemmed	We examine the variation in the radius of the auroral oval, as measured from auroral images gathered by the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft, in response to solar wind inputs measured by the Advanced Composition Explorer (ACE) spacecraft for the two year interval June 2000 to May 2002. Our main finding is that the oval radius increases when the ring current, as measured by the Sym-H index, is intensified during geomagnetic storms. We discuss our findings within the context of the expanding/contracting polar cap paradigm, in terms of a modification of substorm onset conditions by the magnetic perturbation associated with the ring current.
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title_short	Influences on the radius of the auroral oval
url	https://doi.org/10.5194/angeo-27-2913-2009 https://doaj.org/article/0d8ffaaac15c4ba1bfed78b4a76567f3 https://www.ann-geophys.net/27/2913/2009/angeo-27-2913-2009.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576
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score	7.400978

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Influences on the radius of the auroral oval

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