Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction

Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential &...
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Autor*in:	S. E. Milan [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2004

Übergeordnetes Werk:	In: Annales Geophysicae - Copernicus Publications, 2002, 22(2004), Seite 3771-3777
Übergeordnetes Werk:	volume:22 ; year:2004 ; pages:3771-3777

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

DOI / URN:	10.5194/angeo-22-3771-2004

Katalog-ID:	DOAJ002840677

Internformat


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245	1	0	\|a Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction
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520			\|a Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<.
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allfields	10.5194/angeo-22-3771-2004 doi (DE-627)DOAJ002840677 (DE-599)DOAJ151ea69ad452443a85d787120687e9ad DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<. Science Q Physics Geophysics. Cosmic physics In Annales Geophysicae Copernicus Publications, 2002 22(2004), Seite 3771-3777 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:22 year:2004 pages:3771-3777 https://doi.org/10.5194/angeo-22-3771-2004 kostenfrei https://doaj.org/article/151ea69ad452443a85d787120687e9ad kostenfrei https://www.ann-geophys.net/22/3771/2004/angeo-22-3771-2004.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 22 2004 3771-3777
spelling	10.5194/angeo-22-3771-2004 doi (DE-627)DOAJ002840677 (DE-599)DOAJ151ea69ad452443a85d787120687e9ad DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<. Science Q Physics Geophysics. Cosmic physics In Annales Geophysicae Copernicus Publications, 2002 22(2004), Seite 3771-3777 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:22 year:2004 pages:3771-3777 https://doi.org/10.5194/angeo-22-3771-2004 kostenfrei https://doaj.org/article/151ea69ad452443a85d787120687e9ad kostenfrei https://www.ann-geophys.net/22/3771/2004/angeo-22-3771-2004.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 22 2004 3771-3777
allfields_unstemmed	10.5194/angeo-22-3771-2004 doi (DE-627)DOAJ002840677 (DE-599)DOAJ151ea69ad452443a85d787120687e9ad DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<. Science Q Physics Geophysics. Cosmic physics In Annales Geophysicae Copernicus Publications, 2002 22(2004), Seite 3771-3777 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:22 year:2004 pages:3771-3777 https://doi.org/10.5194/angeo-22-3771-2004 kostenfrei https://doaj.org/article/151ea69ad452443a85d787120687e9ad kostenfrei https://www.ann-geophys.net/22/3771/2004/angeo-22-3771-2004.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 22 2004 3771-3777
allfieldsGer	10.5194/angeo-22-3771-2004 doi (DE-627)DOAJ002840677 (DE-599)DOAJ151ea69ad452443a85d787120687e9ad DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<. Science Q Physics Geophysics. Cosmic physics In Annales Geophysicae Copernicus Publications, 2002 22(2004), Seite 3771-3777 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:22 year:2004 pages:3771-3777 https://doi.org/10.5194/angeo-22-3771-2004 kostenfrei https://doaj.org/article/151ea69ad452443a85d787120687e9ad kostenfrei https://www.ann-geophys.net/22/3771/2004/angeo-22-3771-2004.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 22 2004 3771-3777
allfieldsSound	10.5194/angeo-22-3771-2004 doi (DE-627)DOAJ002840677 (DE-599)DOAJ151ea69ad452443a85d787120687e9ad DE-627 ger DE-627 rakwb eng QC1-999 QC801-809 S. E. Milan verfasserin aut Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction 2004 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<. Science Q Physics Geophysics. Cosmic physics In Annales Geophysicae Copernicus Publications, 2002 22(2004), Seite 3771-3777 (DE-627)25338981X (DE-600)1458425-6 14320576 nnns volume:22 year:2004 pages:3771-3777 https://doi.org/10.5194/angeo-22-3771-2004 kostenfrei https://doaj.org/article/151ea69ad452443a85d787120687e9ad kostenfrei https://www.ann-geophys.net/22/3771/2004/angeo-22-3771-2004.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 22 2004 3771-3777
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callnumber-first	Q - Science
author	S. E. Milan
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title	Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction
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title_sort	dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction
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title_auth	Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction
abstract	Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<.
abstractGer	Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<.
abstract_unstemmed	Observations of changes in size of the ionospheric polar cap allow the dayside and nightside reconnection rates to be quantified. From these it is straightforward to estimate the rate of antisunward transport of magnetic flux across the polar regions, quantified by the cross polar cap potential Φ<sub<PC</sub<. When correlated with upstream measurements of the north-south component of the IMF, Φ<sub<PC</sub< is found to increase for more negative <i<B<sub<z</sub<</i<, as expected. However, we also find that Φ<sub<PC</sub< does not, on average, decrease to zero, even for strongly northward IMF. In the past this has been interpreted as evidence for a viscous interaction between the magnetosheath flow and the outer boundaries of the magnetosphere. In contrast, we show that this is the consequence of flows excited by tail reconnection, which is inherently uncorrelated with IMF <i<B<sub<z</sub<</i<.
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title_short	Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction
url	https://doi.org/10.5194/angeo-22-3771-2004 https://doaj.org/article/151ea69ad452443a85d787120687e9ad https://www.ann-geophys.net/22/3771/2004/angeo-22-3771-2004.pdf https://doaj.org/toc/0992-7689 https://doaj.org/toc/1432-0576
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Dayside and nightside contributions to the cross polar cap potential: placing an upper limit on a viscous-like interaction

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