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] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021 |
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| Schlagwörter: |
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| Anmerkung: |
© The Author(s) 2021 |
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| Übergeordnetes Werk: |
Enthalten in: Space science reviews - Springer Netherlands, 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: |
OLC2122862378 |
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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. | ||
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| 650 | 4 | |a Magnetohydrodynamic waves | |
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10.1007/s11214-021-00790-2 doi (DE-627)OLC2122862378 (DE-He213)s11214-021-00790-2-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Zaqarashvili, T. V. verfasserin (orcid)0000-0001-5015-5762 aut Rossby Waves in Astrophysics 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 Solar system planets Sun Stars Astrophysical discs Magnetohydrodynamic waves Albekioni, M. aut Ballester, J. L. (orcid)0000-0001-8921-9225 aut Bekki, Y. aut Biancofiore, L. (orcid)0000-0001-7159-7965 aut Birch, A. C. aut Dikpati, M. (orcid)0000-0002-2227-0488 aut Gizon, L. aut Gurgenashvili, E. aut Heifetz, E. (orcid)0000-0002-3584-3978 aut Lanza, A. F. (orcid)0000-0001-5928-7251 aut McIntosh, S. W. aut Ofman, L. aut Oliver, R. (orcid)0000-0003-4162-7240 aut Proxauf, B. aut Umurhan, O. M. aut Yellin-Bergovoy, R. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 19. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:19 month:01 https://doi.org/10.1007/s11214-021-00790-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 19 01 |
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10.1007/s11214-021-00790-2 doi (DE-627)OLC2122862378 (DE-He213)s11214-021-00790-2-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Zaqarashvili, T. V. verfasserin (orcid)0000-0001-5015-5762 aut Rossby Waves in Astrophysics 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 Solar system planets Sun Stars Astrophysical discs Magnetohydrodynamic waves Albekioni, M. aut Ballester, J. L. (orcid)0000-0001-8921-9225 aut Bekki, Y. aut Biancofiore, L. (orcid)0000-0001-7159-7965 aut Birch, A. C. aut Dikpati, M. (orcid)0000-0002-2227-0488 aut Gizon, L. aut Gurgenashvili, E. aut Heifetz, E. (orcid)0000-0002-3584-3978 aut Lanza, A. F. (orcid)0000-0001-5928-7251 aut McIntosh, S. W. aut Ofman, L. aut Oliver, R. (orcid)0000-0003-4162-7240 aut Proxauf, B. aut Umurhan, O. M. aut Yellin-Bergovoy, R. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 19. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:19 month:01 https://doi.org/10.1007/s11214-021-00790-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 19 01 |
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10.1007/s11214-021-00790-2 doi (DE-627)OLC2122862378 (DE-He213)s11214-021-00790-2-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Zaqarashvili, T. V. verfasserin (orcid)0000-0001-5015-5762 aut Rossby Waves in Astrophysics 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 Solar system planets Sun Stars Astrophysical discs Magnetohydrodynamic waves Albekioni, M. aut Ballester, J. L. (orcid)0000-0001-8921-9225 aut Bekki, Y. aut Biancofiore, L. (orcid)0000-0001-7159-7965 aut Birch, A. C. aut Dikpati, M. (orcid)0000-0002-2227-0488 aut Gizon, L. aut Gurgenashvili, E. aut Heifetz, E. (orcid)0000-0002-3584-3978 aut Lanza, A. F. (orcid)0000-0001-5928-7251 aut McIntosh, S. W. aut Ofman, L. aut Oliver, R. (orcid)0000-0003-4162-7240 aut Proxauf, B. aut Umurhan, O. M. aut Yellin-Bergovoy, R. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 19. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:19 month:01 https://doi.org/10.1007/s11214-021-00790-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 19 01 |
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10.1007/s11214-021-00790-2 doi (DE-627)OLC2122862378 (DE-He213)s11214-021-00790-2-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Zaqarashvili, T. V. verfasserin (orcid)0000-0001-5015-5762 aut Rossby Waves in Astrophysics 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 Solar system planets Sun Stars Astrophysical discs Magnetohydrodynamic waves Albekioni, M. aut Ballester, J. L. (orcid)0000-0001-8921-9225 aut Bekki, Y. aut Biancofiore, L. (orcid)0000-0001-7159-7965 aut Birch, A. C. aut Dikpati, M. (orcid)0000-0002-2227-0488 aut Gizon, L. aut Gurgenashvili, E. aut Heifetz, E. (orcid)0000-0002-3584-3978 aut Lanza, A. F. (orcid)0000-0001-5928-7251 aut McIntosh, S. W. aut Ofman, L. aut Oliver, R. (orcid)0000-0003-4162-7240 aut Proxauf, B. aut Umurhan, O. M. aut Yellin-Bergovoy, R. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 19. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:19 month:01 https://doi.org/10.1007/s11214-021-00790-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 19 01 |
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10.1007/s11214-021-00790-2 doi (DE-627)OLC2122862378 (DE-He213)s11214-021-00790-2-p DE-627 ger DE-627 rakwb eng 600 VZ 16,12 ssgn Zaqarashvili, T. V. verfasserin (orcid)0000-0001-5015-5762 aut Rossby Waves in Astrophysics 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 Solar system planets Sun Stars Astrophysical discs Magnetohydrodynamic waves Albekioni, M. aut Ballester, J. L. (orcid)0000-0001-8921-9225 aut Bekki, Y. aut Biancofiore, L. (orcid)0000-0001-7159-7965 aut Birch, A. C. aut Dikpati, M. (orcid)0000-0002-2227-0488 aut Gizon, L. aut Gurgenashvili, E. aut Heifetz, E. (orcid)0000-0002-3584-3978 aut Lanza, A. F. (orcid)0000-0001-5928-7251 aut McIntosh, S. W. aut Ofman, L. aut Oliver, R. (orcid)0000-0003-4162-7240 aut Proxauf, B. aut Umurhan, O. M. aut Yellin-Bergovoy, R. aut Enthalten in Space science reviews Springer Netherlands, 1962 217(2021), 1 vom: 19. Jan. (DE-627)129086606 (DE-600)4860-4 (DE-576)014420724 0038-6308 nnns volume:217 year:2021 number:1 day:19 month:01 https://doi.org/10.1007/s11214-021-00790-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-AST SSG-OPC-AST GBV_ILN_47 AR 217 2021 1 19 01 |
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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. © The Author(s) 2021 |
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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. © The Author(s) 2021 |
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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. © The Author(s) 2021 |
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