Dispersion and stability of waves in plasmas in the presence of a coriolis force
Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermiti...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Verheest, Frank [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1974 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1974 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 28(1974), 1 vom: Mai, Seite 91-99 |
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| Übergeordnetes Werk: |
volume:28 ; year:1974 ; number:1 ; month:05 ; pages:91-99 |
| Links: |
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| DOI / URN: |
10.1007/BF00642239 |
|---|
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OLC2066121436 |
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| 520 | |a Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. | ||
| 650 | 4 | |a Magnetic Field | |
| 650 | 4 | |a Thermal Effect | |
| 650 | 4 | |a External Magnetic Field | |
| 650 | 4 | |a Rotation Axis | |
| 650 | 4 | |a Static Magnetic Field | |
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10.1007/BF00642239 doi (DE-627)OLC2066121436 (DE-He213)BF00642239-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Verheest, Frank verfasserin aut Dispersion and stability of waves in plasmas in the presence of a coriolis force 1974 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1974 Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. Magnetic Field Thermal Effect External Magnetic Field Rotation Axis Static Magnetic Field Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 28(1974), 1 vom: Mai, Seite 91-99 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:28 year:1974 number:1 month:05 pages:91-99 https://doi.org/10.1007/BF00642239 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 28 1974 1 05 91-99 |
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10.1007/BF00642239 doi (DE-627)OLC2066121436 (DE-He213)BF00642239-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Verheest, Frank verfasserin aut Dispersion and stability of waves in plasmas in the presence of a coriolis force 1974 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1974 Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. Magnetic Field Thermal Effect External Magnetic Field Rotation Axis Static Magnetic Field Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 28(1974), 1 vom: Mai, Seite 91-99 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:28 year:1974 number:1 month:05 pages:91-99 https://doi.org/10.1007/BF00642239 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 28 1974 1 05 91-99 |
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10.1007/BF00642239 doi (DE-627)OLC2066121436 (DE-He213)BF00642239-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Verheest, Frank verfasserin aut Dispersion and stability of waves in plasmas in the presence of a coriolis force 1974 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1974 Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. Magnetic Field Thermal Effect External Magnetic Field Rotation Axis Static Magnetic Field Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 28(1974), 1 vom: Mai, Seite 91-99 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:28 year:1974 number:1 month:05 pages:91-99 https://doi.org/10.1007/BF00642239 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 28 1974 1 05 91-99 |
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10.1007/BF00642239 doi (DE-627)OLC2066121436 (DE-He213)BF00642239-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Verheest, Frank verfasserin aut Dispersion and stability of waves in plasmas in the presence of a coriolis force 1974 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1974 Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. Magnetic Field Thermal Effect External Magnetic Field Rotation Axis Static Magnetic Field Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 28(1974), 1 vom: Mai, Seite 91-99 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:28 year:1974 number:1 month:05 pages:91-99 https://doi.org/10.1007/BF00642239 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 28 1974 1 05 91-99 |
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10.1007/BF00642239 doi (DE-627)OLC2066121436 (DE-He213)BF00642239-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Verheest, Frank verfasserin aut Dispersion and stability of waves in plasmas in the presence of a coriolis force 1974 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1974 Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. Magnetic Field Thermal Effect External Magnetic Field Rotation Axis Static Magnetic Field Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 28(1974), 1 vom: Mai, Seite 91-99 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:28 year:1974 number:1 month:05 pages:91-99 https://doi.org/10.1007/BF00642239 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 28 1974 1 05 91-99 |
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Dispersion and stability of waves in plasmas in the presence of a coriolis force |
| author_sort |
Verheest, Frank |
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Astrophysics and space science |
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Astrophysics and space science |
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eng |
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1974 |
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91 |
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Verheest, Frank |
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Verheest, Frank |
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10.1007/BF00642239 |
| dewey-full |
520 530 620 |
| title_sort |
dispersion and stability of waves in plasmas in the presence of a coriolis force |
| title_auth |
Dispersion and stability of waves in plasmas in the presence of a coriolis force |
| abstract |
Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. © D. Reidel Publishing Company 1974 |
| abstractGer |
Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. © D. Reidel Publishing Company 1974 |
| abstract_unstemmed |
Abstract The dispersion law for the propagation of waves in cold magnetized plasmas is derived for arbitrary directions of the rotation axis with respect to the static magnetic field. The waves are shown to be stable, not only in the case of a cold plasma, but in any plasma case which yields hermitian mobility tensors. An interesting special case is when the rotation and magnetization axes are parallel, because then for suitable values of rotation and external magnetic field the two effects can cancel each other, though only for one plasma species at the time. The rotation thus decisively affects and shifts the number and width of the existing pass- and stop-bands in a magnetized plasma. The inclusion of thermal effects through a scalar barotropic pressure is not nearly as significant. © D. Reidel Publishing Company 1974 |
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| title_short |
Dispersion and stability of waves in plasmas in the presence of a coriolis force |
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