Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms

Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under...
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Autor*in:	Shi, XiaoFei [verfasserIn] Zong, QiuGang [verfasserIn] Wang, YongFu [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2012

Schlagwörter:	pressure-corrected index decay time energy injection

Übergeordnetes Werk:	Enthalten in: Science in China - Heidelberg : Springer, 1997, 55(2012), 10 vom: 01. Aug., Seite 2769-2777
Übergeordnetes Werk:	volume:55 ; year:2012 ; number:10 ; day:01 ; month:08 ; pages:2769-2777

Links:	Volltext

DOI / URN:	10.1007/s11431-012-4989-0

Katalog-ID:	SPR019273436

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520			\|a Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained.
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allfields	10.1007/s11431-012-4989-0 doi (DE-627)SPR019273436 (SPR)s11431-012-4989-0-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Shi, XiaoFei verfasserin aut Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained. pressure-corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 decay time (dpeaa)DE-He213 energy injection (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 10 vom: 01. Aug., Seite 2769-2777 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:10 day:01 month:08 pages:2769-2777 https://dx.doi.org/10.1007/s11431-012-4989-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 10 01 08 2769-2777
spelling	10.1007/s11431-012-4989-0 doi (DE-627)SPR019273436 (SPR)s11431-012-4989-0-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Shi, XiaoFei verfasserin aut Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained. pressure-corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 decay time (dpeaa)DE-He213 energy injection (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 10 vom: 01. Aug., Seite 2769-2777 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:10 day:01 month:08 pages:2769-2777 https://dx.doi.org/10.1007/s11431-012-4989-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 10 01 08 2769-2777
allfields_unstemmed	10.1007/s11431-012-4989-0 doi (DE-627)SPR019273436 (SPR)s11431-012-4989-0-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Shi, XiaoFei verfasserin aut Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained. pressure-corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 decay time (dpeaa)DE-He213 energy injection (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 10 vom: 01. Aug., Seite 2769-2777 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:10 day:01 month:08 pages:2769-2777 https://dx.doi.org/10.1007/s11431-012-4989-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 10 01 08 2769-2777
allfieldsGer	10.1007/s11431-012-4989-0 doi (DE-627)SPR019273436 (SPR)s11431-012-4989-0-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Shi, XiaoFei verfasserin aut Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained. pressure-corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 decay time (dpeaa)DE-He213 energy injection (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 10 vom: 01. Aug., Seite 2769-2777 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:10 day:01 month:08 pages:2769-2777 https://dx.doi.org/10.1007/s11431-012-4989-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 10 01 08 2769-2777
allfieldsSound	10.1007/s11431-012-4989-0 doi (DE-627)SPR019273436 (SPR)s11431-012-4989-0-e DE-627 ger DE-627 rakwb eng 600 ASE 600 ASE 50.00 bkl Shi, XiaoFei verfasserin aut Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained. pressure-corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 decay time (dpeaa)DE-He213 energy injection (dpeaa)DE-He213 Zong, QiuGang verfasserin aut Wang, YongFu verfasserin aut Enthalten in Science in China Heidelberg : Springer, 1997 55(2012), 10 vom: 01. Aug., Seite 2769-2777 (DE-627)385614756 (DE-600)2142897-9 1862-281X nnns volume:55 year:2012 number:10 day:01 month:08 pages:2769-2777 https://dx.doi.org/10.1007/s11431-012-4989-0 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 50.00 ASE AR 55 2012 10 01 08 2769-2777
language	English
source	Enthalten in Science in China 55(2012), 10 vom: 01. Aug., Seite 2769-2777 volume:55 year:2012 number:10 day:01 month:08 pages:2769-2777
sourceStr	Enthalten in Science in China 55(2012), 10 vom: 01. Aug., Seite 2769-2777 volume:55 year:2012 number:10 day:01 month:08 pages:2769-2777
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authorswithroles_txt_mv	Shi, XiaoFei @@aut@@ Zong, QiuGang @@aut@@ Wang, YongFu @@aut@@
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Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. 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author	Shi, XiaoFei
spellingShingle	Shi, XiaoFei ddc 600 bkl 50.00 misc pressure-corrected misc index misc decay time misc energy injection Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms
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topic_title	600 ASE 50.00 bkl Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms pressure-corrected (dpeaa)DE-He213 index (dpeaa)DE-He213 decay time (dpeaa)DE-He213 energy injection (dpeaa)DE-He213
topic	ddc 600 bkl 50.00 misc pressure-corrected misc index misc decay time misc energy injection
topic_unstemmed	ddc 600 bkl 50.00 misc pressure-corrected misc index misc decay time misc energy injection
topic_browse	ddc 600 bkl 50.00 misc pressure-corrected misc index misc decay time misc energy injection
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title	Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms
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title_full	Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms
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journal	Science in China
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author_browse	Shi, XiaoFei Zong, QiuGang Wang, YongFu
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title_sort	comparison between the ring current energy injection and decay under southward and northward imf bz conditions during geomagnetic storms
title_auth	Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms
abstract	Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained.
abstractGer	Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained.
abstract_unstemmed	Abstract The geomagnetic storm is one of the most important geomagnetic disturbance phenomena in the geospace. Many studies assume that input of solar wind energy into the Earth’s ring current only occurs when IMF Bz in GSM coordinates is southward; the ring current energy injection and decay under northward IMF Bz are not well understood and still need further investigation. In this paper, by using the large amount of data from the year 1964 to 2010, we use the empirical phase space analysis method to study the ring current energy injection and decay under northward IMF Bz and compare the results with those under southward IMF Bz condition. We have found that the largest injection Q under northward IMF Bz condition is only 7% of the largest injection under southward IMF Bz, implying that there is a very limit energy injected into the ring current region when IMF Bz is northward. The decay time τ decreases as VBz increases and shows a good linear trend for southward IMF Bz; while for the northward IMF Bz, there is not a clear relation between τ varies and VBz. Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. The statistical results on between the different geomagnetic indices (Dst, Kp, AE) and IMF Bz are also obtained.
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title_short	Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms
url	https://dx.doi.org/10.1007/s11431-012-4989-0
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author2	Zong, QiuGang Wang, YongFu
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doi_str	10.1007/s11431-012-4989-0
up_date	2024-07-04T00:55:04.859Z
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Having taken τ as a function of injection Q instead of VBz, we have obtained the empirical relation of τ with Q for northward and southward IMF Bz conditions: the two categories are further combined together and the empirical relation τ=e(2.6+0.039-Q) is derived. Further, the pressure-corrected Dst formula $Dst^* = Dst - b\sqrt P + c$ is derived for both southward and northward IMF Bz conditions, where the coefficients b and c are 6.9/10.4 and 10.0/15.2 when IMF Bz is southward and northward respectively. 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Comparison between the ring current energy injection and decay under southward and northward IMF Bz conditions during geomagnetic storms

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