Rossby Waves in Astrophysics
Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior,...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Zaqarashvili, T. V. [verfasserIn] Albekioni, M. [verfasserIn] Ballester, J. L. [verfasserIn] Bekki, Y. [verfasserIn] Biancofiore, L. [verfasserIn] Birch, A. C. [verfasserIn] Dikpati, M. [verfasserIn] Gizon, L. [verfasserIn] Gurgenashvili, E. [verfasserIn] Heifetz, E. [verfasserIn] Lanza, A. F. [verfasserIn] McIntosh, S. W. [verfasserIn] Ofman, L. [verfasserIn] Oliver, R. [verfasserIn] Proxauf, B. [verfasserIn] Umurhan, O. M. [verfasserIn] Yellin-Bergovoy, R. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962, 217(2021), 1 vom: 19. Jan. |
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| Übergeordnetes Werk: |
volume:217 ; year:2021 ; number:1 ; day:19 ; month:01 |
| Links: |
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| DOI / URN: |
10.1007/s11214-021-00790-2 |
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| Katalog-ID: |
SPR042754631 |
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| 520 | |a Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. | ||
| 650 | 4 | |a Rossby waves |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Solar system planets |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Sun |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Stars |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Astrophysical discs |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Magnetohydrodynamic waves |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Albekioni, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Ballester, J. L. |e verfasserin |4 aut | |
| 700 | 1 | |a Bekki, Y. |e verfasserin |4 aut | |
| 700 | 1 | |a Biancofiore, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Birch, A. C. |e verfasserin |4 aut | |
| 700 | 1 | |a Dikpati, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Gizon, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Gurgenashvili, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Heifetz, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Lanza, A. F. |e verfasserin |4 aut | |
| 700 | 1 | |a McIntosh, S. W. |e verfasserin |4 aut | |
| 700 | 1 | |a Ofman, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Oliver, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Proxauf, B. |e verfasserin |4 aut | |
| 700 | 1 | |a Umurhan, O. M. |e verfasserin |4 aut | |
| 700 | 1 | |a Yellin-Bergovoy, R. |e verfasserin |4 aut | |
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10.1007/s11214-021-00790-2 doi (DE-627)SPR042754631 (DE-599)SPRs11214-021-00790-2-e (SPR)s11214-021-00790-2-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Zaqarashvili, T. V. verfasserin aut Rossby Waves in Astrophysics 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. Rossby waves (dpeaa)DE-He213 Solar system planets (dpeaa)DE-He213 Sun (dpeaa)DE-He213 Stars (dpeaa)DE-He213 Astrophysical discs (dpeaa)DE-He213 Magnetohydrodynamic waves (dpeaa)DE-He213 Albekioni, M. verfasserin aut Ballester, J. L. verfasserin aut Bekki, Y. verfasserin aut Biancofiore, L. verfasserin aut Birch, A. C. verfasserin aut Dikpati, M. verfasserin aut Gizon, L. verfasserin aut Gurgenashvili, E. verfasserin aut Heifetz, E. verfasserin aut Lanza, A. F. verfasserin aut McIntosh, S. W. verfasserin aut Ofman, L. verfasserin aut Oliver, R. verfasserin aut Proxauf, B. verfasserin aut Umurhan, O. M. verfasserin aut Yellin-Bergovoy, R. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 217(2021), 1 vom: 19. Jan. (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:217 year:2021 number:1 day:19 month:01 https://dx.doi.org/10.1007/s11214-021-00790-2 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 217 2021 1 19 01 |
| spelling |
10.1007/s11214-021-00790-2 doi (DE-627)SPR042754631 (DE-599)SPRs11214-021-00790-2-e (SPR)s11214-021-00790-2-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Zaqarashvili, T. V. verfasserin aut Rossby Waves in Astrophysics 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. Rossby waves (dpeaa)DE-He213 Solar system planets (dpeaa)DE-He213 Sun (dpeaa)DE-He213 Stars (dpeaa)DE-He213 Astrophysical discs (dpeaa)DE-He213 Magnetohydrodynamic waves (dpeaa)DE-He213 Albekioni, M. verfasserin aut Ballester, J. L. verfasserin aut Bekki, Y. verfasserin aut Biancofiore, L. verfasserin aut Birch, A. C. verfasserin aut Dikpati, M. verfasserin aut Gizon, L. verfasserin aut Gurgenashvili, E. verfasserin aut Heifetz, E. verfasserin aut Lanza, A. F. verfasserin aut McIntosh, S. W. verfasserin aut Ofman, L. verfasserin aut Oliver, R. verfasserin aut Proxauf, B. verfasserin aut Umurhan, O. M. verfasserin aut Yellin-Bergovoy, R. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 217(2021), 1 vom: 19. Jan. (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:217 year:2021 number:1 day:19 month:01 https://dx.doi.org/10.1007/s11214-021-00790-2 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 217 2021 1 19 01 |
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10.1007/s11214-021-00790-2 doi (DE-627)SPR042754631 (DE-599)SPRs11214-021-00790-2-e (SPR)s11214-021-00790-2-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Zaqarashvili, T. V. verfasserin aut Rossby Waves in Astrophysics 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. Rossby waves (dpeaa)DE-He213 Solar system planets (dpeaa)DE-He213 Sun (dpeaa)DE-He213 Stars (dpeaa)DE-He213 Astrophysical discs (dpeaa)DE-He213 Magnetohydrodynamic waves (dpeaa)DE-He213 Albekioni, M. verfasserin aut Ballester, J. L. verfasserin aut Bekki, Y. verfasserin aut Biancofiore, L. verfasserin aut Birch, A. C. verfasserin aut Dikpati, M. verfasserin aut Gizon, L. verfasserin aut Gurgenashvili, E. verfasserin aut Heifetz, E. verfasserin aut Lanza, A. F. verfasserin aut McIntosh, S. W. verfasserin aut Ofman, L. verfasserin aut Oliver, R. verfasserin aut Proxauf, B. verfasserin aut Umurhan, O. M. verfasserin aut Yellin-Bergovoy, R. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 217(2021), 1 vom: 19. Jan. (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:217 year:2021 number:1 day:19 month:01 https://dx.doi.org/10.1007/s11214-021-00790-2 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 217 2021 1 19 01 |
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10.1007/s11214-021-00790-2 doi (DE-627)SPR042754631 (DE-599)SPRs11214-021-00790-2-e (SPR)s11214-021-00790-2-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Zaqarashvili, T. V. verfasserin aut Rossby Waves in Astrophysics 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. Rossby waves (dpeaa)DE-He213 Solar system planets (dpeaa)DE-He213 Sun (dpeaa)DE-He213 Stars (dpeaa)DE-He213 Astrophysical discs (dpeaa)DE-He213 Magnetohydrodynamic waves (dpeaa)DE-He213 Albekioni, M. verfasserin aut Ballester, J. L. verfasserin aut Bekki, Y. verfasserin aut Biancofiore, L. verfasserin aut Birch, A. C. verfasserin aut Dikpati, M. verfasserin aut Gizon, L. verfasserin aut Gurgenashvili, E. verfasserin aut Heifetz, E. verfasserin aut Lanza, A. F. verfasserin aut McIntosh, S. W. verfasserin aut Ofman, L. verfasserin aut Oliver, R. verfasserin aut Proxauf, B. verfasserin aut Umurhan, O. M. verfasserin aut Yellin-Bergovoy, R. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 217(2021), 1 vom: 19. Jan. (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:217 year:2021 number:1 day:19 month:01 https://dx.doi.org/10.1007/s11214-021-00790-2 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 217 2021 1 19 01 |
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10.1007/s11214-021-00790-2 doi (DE-627)SPR042754631 (DE-599)SPRs11214-021-00790-2-e (SPR)s11214-021-00790-2-e DE-627 ger DE-627 rakwb eng 600 ASE 39.00 bkl Zaqarashvili, T. V. verfasserin aut Rossby Waves in Astrophysics 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. Rossby waves (dpeaa)DE-He213 Solar system planets (dpeaa)DE-He213 Sun (dpeaa)DE-He213 Stars (dpeaa)DE-He213 Astrophysical discs (dpeaa)DE-He213 Magnetohydrodynamic waves (dpeaa)DE-He213 Albekioni, M. verfasserin aut Ballester, J. L. verfasserin aut Bekki, Y. verfasserin aut Biancofiore, L. verfasserin aut Birch, A. C. verfasserin aut Dikpati, M. verfasserin aut Gizon, L. verfasserin aut Gurgenashvili, E. verfasserin aut Heifetz, E. verfasserin aut Lanza, A. F. verfasserin aut McIntosh, S. W. verfasserin aut Ofman, L. verfasserin aut Oliver, R. verfasserin aut Proxauf, B. verfasserin aut Umurhan, O. M. verfasserin aut Yellin-Bergovoy, R. verfasserin aut Enthalten in Space science reviews Dordrecht [u.a.] : Springer Science + Business Media B.V, 1962 217(2021), 1 vom: 19. Jan. (DE-627)315621222 (DE-600)2017804-9 1572-9672 nnns volume:217 year:2021 number:1 day:19 month:01 https://dx.doi.org/10.1007/s11214-021-00790-2 kostenfrei Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 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_4326 GBV_ILN_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 217 2021 1 19 01 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR042754631</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220111053834.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">210120s2021 xx |||||o 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11214-021-00790-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR042754631</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)SPRs11214-021-00790-2-e</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)s11214-021-00790-2-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">600</subfield><subfield code="q">ASE</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">39.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Zaqarashvili, T. V.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Rossby Waves in Astrophysics</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2021</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. 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|
| author |
Zaqarashvili, T. V. |
| spellingShingle |
Zaqarashvili, T. V. ddc 600 bkl 39.00 misc Rossby waves misc Solar system planets misc Sun misc Stars misc Astrophysical discs misc Magnetohydrodynamic waves Rossby Waves in Astrophysics |
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Zaqarashvili, T. V. |
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electronic Article |
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600 - Technology |
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1572-9672 |
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600 ASE 39.00 bkl Rossby Waves in Astrophysics Rossby waves (dpeaa)DE-He213 Solar system planets (dpeaa)DE-He213 Sun (dpeaa)DE-He213 Stars (dpeaa)DE-He213 Astrophysical discs (dpeaa)DE-He213 Magnetohydrodynamic waves (dpeaa)DE-He213 |
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ddc 600 bkl 39.00 misc Rossby waves misc Solar system planets misc Sun misc Stars misc Astrophysical discs misc Magnetohydrodynamic waves |
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ddc 600 bkl 39.00 misc Rossby waves misc Solar system planets misc Sun misc Stars misc Astrophysical discs misc Magnetohydrodynamic waves |
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ddc 600 bkl 39.00 misc Rossby waves misc Solar system planets misc Sun misc Stars misc Astrophysical discs misc Magnetohydrodynamic waves |
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Elektronische Aufsätze Aufsätze Elektronische Ressource |
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Rossby Waves in Astrophysics |
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Zaqarashvili, T. V. |
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Zaqarashvili, T. V. Albekioni, M. Ballester, J. L. Bekki, Y. Biancofiore, L. Birch, A. C. Dikpati, M. Gizon, L. Gurgenashvili, E. Heifetz, E. Lanza, A. F. McIntosh, S. W. Ofman, L. Oliver, R. Proxauf, B. Umurhan, O. M. Yellin-Bergovoy, R. |
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Rossby Waves in Astrophysics |
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Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. |
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Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. |
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Abstract Rossby waves are a pervasive feature of the large-scale motions of the Earth’s atmosphere and oceans. These waves (also known as planetary waves and r-modes) also play an important role in the large-scale dynamics of different astrophysical objects such as the solar atmosphere and interior, astrophysical discs, rapidly rotating stars, planetary and exoplanetary atmospheres. This paper provides a review of theoretical and observational aspects of Rossby waves on different spatial and temporal scales in various astrophysical settings. The physical role played by Rossby-type waves and associated instabilities is discussed in the context of solar and stellar magnetic activity, angular momentum transport in astrophysical discs, planet formation, and other astrophysical processes. Possible directions of future research in theoretical and observational aspects of astrophysical Rossby waves are outlined. |
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| score |
7.3993473 |