Quasi-static evolution in multiple arcades
Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade s...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Sciffer, Murray [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1996 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1996 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 166(1996), 1 vom: Juni, Seite 173-193 |
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| Übergeordnetes Werk: |
volume:166 ; year:1996 ; number:1 ; month:06 ; pages:173-193 |
| Links: |
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| DOI / URN: |
10.1007/BF00179361 |
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OLC2033580024 |
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| 520 | |a Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. | ||
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| 650 | 4 | |a Coronal Mass Ejection | |
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10.1007/BF00179361 doi (DE-627)OLC2033580024 (DE-He213)BF00179361-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Sciffer, Murray verfasserin aut Quasi-static evolution in multiple arcades 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. Magnetic Field Equilibrium State Equilibrium Equation Coronal Mass Ejection Dynamical Evolution Enthalten in Solar physics Kluwer Academic Publishers, 1967 166(1996), 1 vom: Juni, Seite 173-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:166 year:1996 number:1 month:06 pages:173-193 https://doi.org/10.1007/BF00179361 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 166 1996 1 06 173-193 |
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10.1007/BF00179361 doi (DE-627)OLC2033580024 (DE-He213)BF00179361-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Sciffer, Murray verfasserin aut Quasi-static evolution in multiple arcades 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. Magnetic Field Equilibrium State Equilibrium Equation Coronal Mass Ejection Dynamical Evolution Enthalten in Solar physics Kluwer Academic Publishers, 1967 166(1996), 1 vom: Juni, Seite 173-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:166 year:1996 number:1 month:06 pages:173-193 https://doi.org/10.1007/BF00179361 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 166 1996 1 06 173-193 |
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10.1007/BF00179361 doi (DE-627)OLC2033580024 (DE-He213)BF00179361-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Sciffer, Murray verfasserin aut Quasi-static evolution in multiple arcades 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. Magnetic Field Equilibrium State Equilibrium Equation Coronal Mass Ejection Dynamical Evolution Enthalten in Solar physics Kluwer Academic Publishers, 1967 166(1996), 1 vom: Juni, Seite 173-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:166 year:1996 number:1 month:06 pages:173-193 https://doi.org/10.1007/BF00179361 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 166 1996 1 06 173-193 |
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10.1007/BF00179361 doi (DE-627)OLC2033580024 (DE-He213)BF00179361-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Sciffer, Murray verfasserin aut Quasi-static evolution in multiple arcades 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. Magnetic Field Equilibrium State Equilibrium Equation Coronal Mass Ejection Dynamical Evolution Enthalten in Solar physics Kluwer Academic Publishers, 1967 166(1996), 1 vom: Juni, Seite 173-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:166 year:1996 number:1 month:06 pages:173-193 https://doi.org/10.1007/BF00179361 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 166 1996 1 06 173-193 |
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10.1007/BF00179361 doi (DE-627)OLC2033580024 (DE-He213)BF00179361-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Sciffer, Murray verfasserin aut Quasi-static evolution in multiple arcades 1996 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1996 Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. Magnetic Field Equilibrium State Equilibrium Equation Coronal Mass Ejection Dynamical Evolution Enthalten in Solar physics Kluwer Academic Publishers, 1967 166(1996), 1 vom: Juni, Seite 173-193 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:166 year:1996 number:1 month:06 pages:173-193 https://doi.org/10.1007/BF00179361 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4306 AR 166 1996 1 06 173-193 |
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Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. © Kluwer Academic Publishers 1996 |
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Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. © Kluwer Academic Publishers 1996 |
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Abstract The slow dynamical evolution of solar atmospheric magnetic field structures via the equilibrium equation has been the subject of a number of investigations. In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. When new flux emerges from the photospheric boundary under a pre-existing magnetic arcade the results suggest that such a mechanism will initiate coronal mass ejection. © Kluwer Academic Publishers 1996 |
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In many of these studies the quasi-static evolution of the field and the associated plasma has been investigated for a single arcade structure. In this paper we present results for multiple arcade structures. For multiple arcades we do not find bifurcations and the consequent multiple solutions as the field is evolved through a sequence of equilibrium states, in contrast to the findings for single arcade. Further we show that particular polarity arrangements within a pair of arcade structures lead to quite different topologies of the field as it is evolved. 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