Latitudinal shift and tilt of the ring current during magnetic storms

Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Chen, Bo [verfasserIn] Xu, WenYao [verfasserIn] Chen, GengXiong [verfasserIn] Du, AiMin [verfasserIn] Wu, YingYan [verfasserIn] Liu, XiaoCan [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2008

Schlagwörter:	ring current geomagnetic inversion configuration tilt and latitude shift magnetic storms

Übergeordnetes Werk:	Enthalten in: Chinese science bulletin - Beijing, China : Chinese Acad. of Sciences, 1997, 54(2008), 1 vom: 10. Okt., Seite 95-103
Übergeordnetes Werk:	volume:54 ; year:2008 ; number:1 ; day:10 ; month:10 ; pages:95-103

Links:	Volltext

DOI / URN:	10.1007/s11434-008-0364-8

Katalog-ID:	SPR019381964

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520			\|a Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations.
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allfields	10.1007/s11434-008-0364-8 doi (DE-627)SPR019381964 (SPR)s11434-008-0364-8-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Chen, Bo verfasserin aut Latitudinal shift and tilt of the ring current during magnetic storms 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations. ring current (dpeaa)DE-He213 geomagnetic inversion (dpeaa)DE-He213 configuration (dpeaa)DE-He213 tilt and latitude shift (dpeaa)DE-He213 magnetic storms (dpeaa)DE-He213 Xu, WenYao verfasserin aut Chen, GengXiong verfasserin aut Du, AiMin verfasserin aut Wu, YingYan verfasserin aut Liu, XiaoCan verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 54(2008), 1 vom: 10. Okt., Seite 95-103 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:54 year:2008 number:1 day:10 month:10 pages:95-103 https://dx.doi.org/10.1007/s11434-008-0364-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_161 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4313 GBV_ILN_4328 GBV_ILN_4333 30.00 ASE AR 54 2008 1 10 10 95-103
spelling	10.1007/s11434-008-0364-8 doi (DE-627)SPR019381964 (SPR)s11434-008-0364-8-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Chen, Bo verfasserin aut Latitudinal shift and tilt of the ring current during magnetic storms 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations. ring current (dpeaa)DE-He213 geomagnetic inversion (dpeaa)DE-He213 configuration (dpeaa)DE-He213 tilt and latitude shift (dpeaa)DE-He213 magnetic storms (dpeaa)DE-He213 Xu, WenYao verfasserin aut Chen, GengXiong verfasserin aut Du, AiMin verfasserin aut Wu, YingYan verfasserin aut Liu, XiaoCan verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 54(2008), 1 vom: 10. Okt., Seite 95-103 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:54 year:2008 number:1 day:10 month:10 pages:95-103 https://dx.doi.org/10.1007/s11434-008-0364-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_161 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4313 GBV_ILN_4328 GBV_ILN_4333 30.00 ASE AR 54 2008 1 10 10 95-103
allfields_unstemmed	10.1007/s11434-008-0364-8 doi (DE-627)SPR019381964 (SPR)s11434-008-0364-8-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Chen, Bo verfasserin aut Latitudinal shift and tilt of the ring current during magnetic storms 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations. ring current (dpeaa)DE-He213 geomagnetic inversion (dpeaa)DE-He213 configuration (dpeaa)DE-He213 tilt and latitude shift (dpeaa)DE-He213 magnetic storms (dpeaa)DE-He213 Xu, WenYao verfasserin aut Chen, GengXiong verfasserin aut Du, AiMin verfasserin aut Wu, YingYan verfasserin aut Liu, XiaoCan verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 54(2008), 1 vom: 10. Okt., Seite 95-103 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:54 year:2008 number:1 day:10 month:10 pages:95-103 https://dx.doi.org/10.1007/s11434-008-0364-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_161 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4313 GBV_ILN_4328 GBV_ILN_4333 30.00 ASE AR 54 2008 1 10 10 95-103
allfieldsGer	10.1007/s11434-008-0364-8 doi (DE-627)SPR019381964 (SPR)s11434-008-0364-8-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Chen, Bo verfasserin aut Latitudinal shift and tilt of the ring current during magnetic storms 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations. ring current (dpeaa)DE-He213 geomagnetic inversion (dpeaa)DE-He213 configuration (dpeaa)DE-He213 tilt and latitude shift (dpeaa)DE-He213 magnetic storms (dpeaa)DE-He213 Xu, WenYao verfasserin aut Chen, GengXiong verfasserin aut Du, AiMin verfasserin aut Wu, YingYan verfasserin aut Liu, XiaoCan verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 54(2008), 1 vom: 10. Okt., Seite 95-103 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:54 year:2008 number:1 day:10 month:10 pages:95-103 https://dx.doi.org/10.1007/s11434-008-0364-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_161 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4313 GBV_ILN_4328 GBV_ILN_4333 30.00 ASE AR 54 2008 1 10 10 95-103
allfieldsSound	10.1007/s11434-008-0364-8 doi (DE-627)SPR019381964 (SPR)s11434-008-0364-8-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Chen, Bo verfasserin aut Latitudinal shift and tilt of the ring current during magnetic storms 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations. ring current (dpeaa)DE-He213 geomagnetic inversion (dpeaa)DE-He213 configuration (dpeaa)DE-He213 tilt and latitude shift (dpeaa)DE-He213 magnetic storms (dpeaa)DE-He213 Xu, WenYao verfasserin aut Chen, GengXiong verfasserin aut Du, AiMin verfasserin aut Wu, YingYan verfasserin aut Liu, XiaoCan verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 54(2008), 1 vom: 10. Okt., Seite 95-103 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:54 year:2008 number:1 day:10 month:10 pages:95-103 https://dx.doi.org/10.1007/s11434-008-0364-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_40 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_110 GBV_ILN_120 GBV_ILN_161 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4313 GBV_ILN_4328 GBV_ILN_4333 30.00 ASE AR 54 2008 1 10 10 95-103
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However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. 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author	Chen, Bo
spellingShingle	Chen, Bo ddc 500 bkl 30.00 misc ring current misc geomagnetic inversion misc configuration misc tilt and latitude shift misc magnetic storms Latitudinal shift and tilt of the ring current during magnetic storms
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topic_title	500 ASE 30.00 bkl Latitudinal shift and tilt of the ring current during magnetic storms ring current (dpeaa)DE-He213 geomagnetic inversion (dpeaa)DE-He213 configuration (dpeaa)DE-He213 tilt and latitude shift (dpeaa)DE-He213 magnetic storms (dpeaa)DE-He213
topic	ddc 500 bkl 30.00 misc ring current misc geomagnetic inversion misc configuration misc tilt and latitude shift misc magnetic storms
topic_unstemmed	ddc 500 bkl 30.00 misc ring current misc geomagnetic inversion misc configuration misc tilt and latitude shift misc magnetic storms
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title	Latitudinal shift and tilt of the ring current during magnetic storms
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title_full	Latitudinal shift and tilt of the ring current during magnetic storms
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author_browse	Chen, Bo Xu, WenYao Chen, GengXiong Du, AiMin Wu, YingYan Liu, XiaoCan
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title_sort	latitudinal shift and tilt of the ring current during magnetic storms
title_auth	Latitudinal shift and tilt of the ring current during magnetic storms
abstract	Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations.
abstractGer	Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations.
abstract_unstemmed	Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. The ground disturbed field distribution should be improved as ΔHk = ΔHmaxcos(ϕk–δ), which agree well with the geomagnetic observations.
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title_short	Latitudinal shift and tilt of the ring current during magnetic storms
url	https://dx.doi.org/10.1007/s11434-008-0364-8
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author2	Xu, WenYao Chen, GengXiong Du, AiMin Wu, YingYan Liu, XiaoCan
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up_date	2024-07-04T01:20:38.631Z
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fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR019381964</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111065823.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201006s2008 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11434-008-0364-8</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR019381964</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11434-008-0364-8-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">500</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">30.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Chen, Bo</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Latitudinal shift and tilt of the ring current during magnetic storms</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2008</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The equatorial ring current (ERC) theory suggested that the distribution of global disturbed horizontal geomagnetic field only depends on the cosine of station’s latitude. However, we always observe a larger ΔH at higher latitude stations than lower ones, implying that the ERC could tilt or/and shift with respect to the equatorial plane during intense storms. In this paper, we analyze 11 intense magnetic storms from 2000 to 2004, and introduce two configurational factors to characterize the topology of storm time ring current. The results show that ERC has occasionally deviated off equatorial plane with both tilt angle δt≈13°–25° and latitude shift δs≈0°–21.8°. 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Latitudinal shift and tilt of the ring current during magnetic storms

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