Wave-trains in the solar wind
Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation fo...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Olbers, Dirk J. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1973 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1973 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 20(1973), 2 vom: Feb., Seite 373-389 |
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| Übergeordnetes Werk: |
volume:20 ; year:1973 ; number:2 ; month:02 ; pages:373-389 |
| Links: |
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| DOI / URN: |
10.1007/BF00642209 |
|---|
| Katalog-ID: |
OLC2066118834 |
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| 520 | |a Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. | ||
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10.1007/BF00642209 doi (DE-627)OLC2066118834 (DE-He213)BF00642209-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Olbers, Dirk J. verfasserin aut Wave-trains in the solar wind 1973 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1973 Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. Solar Wind Lower Order Order Approximation Lagrangian Method Lower Order Approximation Richter, Arne K. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 20(1973), 2 vom: Feb., Seite 373-389 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:20 year:1973 number:2 month:02 pages:373-389 https://doi.org/10.1007/BF00642209 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 AR 20 1973 2 02 373-389 |
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10.1007/BF00642209 doi (DE-627)OLC2066118834 (DE-He213)BF00642209-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Olbers, Dirk J. verfasserin aut Wave-trains in the solar wind 1973 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1973 Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. Solar Wind Lower Order Order Approximation Lagrangian Method Lower Order Approximation Richter, Arne K. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 20(1973), 2 vom: Feb., Seite 373-389 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:20 year:1973 number:2 month:02 pages:373-389 https://doi.org/10.1007/BF00642209 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 AR 20 1973 2 02 373-389 |
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10.1007/BF00642209 doi (DE-627)OLC2066118834 (DE-He213)BF00642209-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Olbers, Dirk J. verfasserin aut Wave-trains in the solar wind 1973 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1973 Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. Solar Wind Lower Order Order Approximation Lagrangian Method Lower Order Approximation Richter, Arne K. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 20(1973), 2 vom: Feb., Seite 373-389 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:20 year:1973 number:2 month:02 pages:373-389 https://doi.org/10.1007/BF00642209 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 AR 20 1973 2 02 373-389 |
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10.1007/BF00642209 doi (DE-627)OLC2066118834 (DE-He213)BF00642209-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Olbers, Dirk J. verfasserin aut Wave-trains in the solar wind 1973 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1973 Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. Solar Wind Lower Order Order Approximation Lagrangian Method Lower Order Approximation Richter, Arne K. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 20(1973), 2 vom: Feb., Seite 373-389 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:20 year:1973 number:2 month:02 pages:373-389 https://doi.org/10.1007/BF00642209 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 AR 20 1973 2 02 373-389 |
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10.1007/BF00642209 doi (DE-627)OLC2066118834 (DE-He213)BF00642209-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Olbers, Dirk J. verfasserin aut Wave-trains in the solar wind 1973 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1973 Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. Solar Wind Lower Order Order Approximation Lagrangian Method Lower Order Approximation Richter, Arne K. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 20(1973), 2 vom: Feb., Seite 373-389 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:20 year:1973 number:2 month:02 pages:373-389 https://doi.org/10.1007/BF00642209 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_601 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 AR 20 1973 2 02 373-389 |
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Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. © D. Reidel Publishing Company 1973 |
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Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. © D. Reidel Publishing Company 1973 |
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Abstract The main results of Whitham's averaged Lagrangian method for the treatment of linear wave-trains in a weakly inhomogeneous, moving medium are presented briefly. This method is then applied to an ideal, isotropic, one-fluid plasma which can be taken for the lowest order approximation for the interplanetary solar wind expansion. © D. Reidel Publishing Company 1973 |
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Wave-trains in the solar wind |
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