Plasmasphere Response: Tutorial and Review of Recent Imaging Results
Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion c...
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Gespeichert in:
| Autor*in: |
Goldstein, J. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2006 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science+Business Media, Inc. 2006 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Kluwer Academic Publishers, 1962, 124(2006), 1-4 vom: Juni, Seite 203-216 |
|---|---|
| Übergeordnetes Werk: |
volume:124 ; year:2006 ; number:1-4 ; month:06 ; pages:203-216 |
| Links: |
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| DOI / URN: |
10.1007/s11214-006-9105-y |
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OLC2033691187 |
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| 520 | |a Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. | ||
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10.1007/s11214-006-9105-y doi (DE-627)OLC2033691187 (DE-He213)s11214-006-9105-y-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goldstein, J. verfasserin aut Plasmasphere Response: Tutorial and Review of Recent Imaging Results 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, Inc. 2006 Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. plasmasphere inner magnetosphere imaging erosion electric fields radiation belts Enthalten in Space science reviews Kluwer Academic Publishers, 1962 124(2006), 1-4 vom: Juni, Seite 203-216 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:124 year:2006 number:1-4 month:06 pages:203-216 https://doi.org/10.1007/s11214-006-9105-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 124 2006 1-4 06 203-216 |
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10.1007/s11214-006-9105-y doi (DE-627)OLC2033691187 (DE-He213)s11214-006-9105-y-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goldstein, J. verfasserin aut Plasmasphere Response: Tutorial and Review of Recent Imaging Results 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, Inc. 2006 Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. plasmasphere inner magnetosphere imaging erosion electric fields radiation belts Enthalten in Space science reviews Kluwer Academic Publishers, 1962 124(2006), 1-4 vom: Juni, Seite 203-216 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:124 year:2006 number:1-4 month:06 pages:203-216 https://doi.org/10.1007/s11214-006-9105-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 124 2006 1-4 06 203-216 |
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10.1007/s11214-006-9105-y doi (DE-627)OLC2033691187 (DE-He213)s11214-006-9105-y-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goldstein, J. verfasserin aut Plasmasphere Response: Tutorial and Review of Recent Imaging Results 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, Inc. 2006 Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. plasmasphere inner magnetosphere imaging erosion electric fields radiation belts Enthalten in Space science reviews Kluwer Academic Publishers, 1962 124(2006), 1-4 vom: Juni, Seite 203-216 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:124 year:2006 number:1-4 month:06 pages:203-216 https://doi.org/10.1007/s11214-006-9105-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 124 2006 1-4 06 203-216 |
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10.1007/s11214-006-9105-y doi (DE-627)OLC2033691187 (DE-He213)s11214-006-9105-y-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goldstein, J. verfasserin aut Plasmasphere Response: Tutorial and Review of Recent Imaging Results 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, Inc. 2006 Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. plasmasphere inner magnetosphere imaging erosion electric fields radiation belts Enthalten in Space science reviews Kluwer Academic Publishers, 1962 124(2006), 1-4 vom: Juni, Seite 203-216 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:124 year:2006 number:1-4 month:06 pages:203-216 https://doi.org/10.1007/s11214-006-9105-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 124 2006 1-4 06 203-216 |
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10.1007/s11214-006-9105-y doi (DE-627)OLC2033691187 (DE-He213)s11214-006-9105-y-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Goldstein, J. verfasserin aut Plasmasphere Response: Tutorial and Review of Recent Imaging Results 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science+Business Media, Inc. 2006 Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. plasmasphere inner magnetosphere imaging erosion electric fields radiation belts Enthalten in Space science reviews Kluwer Academic Publishers, 1962 124(2006), 1-4 vom: Juni, Seite 203-216 (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:124 year:2006 number:1-4 month:06 pages:203-216 https://doi.org/10.1007/s11214-006-9105-y lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2279 GBV_ILN_4046 GBV_ILN_4306 GBV_ILN_4700 AR 124 2006 1-4 06 203-216 |
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Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. © Springer Science+Business Media, Inc. 2006 |
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Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. © Springer Science+Business Media, Inc. 2006 |
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Abstract The plasmasphere is the cold, dense innermost region of the magnetosphere that is populated by upflow of ionospheric plasma along geomagnetic field lines. Driven directly by dayside magnetopause reconnection, enhanced sunward convection erodes the outer layers of the plasmasphere. Erosion causes the plasmasphere outer boundary, the plasmapause, to move inward on the nightside and outward on the dayside to form plumes of dense plasma extending sunward into the outer magnetosphere. Coupling between the inner magnetosphere and ionosphere can significantly modify the convection field, either enhancing sunward flows near dusk or shielding them on the night side. The plasmaspheric configuration plays a crucial role in the inner magnetosphere; wave-particle interactions inside the plasmasphere can cause scattering and loss of warmer space plasmas such as the ring current and radiation belts. © Springer Science+Business Media, Inc. 2006 |
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Plasmasphere Response: Tutorial and Review of Recent Imaging Results |
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