Flux Emergence (Theory)
Magnetic flux emergence from the solar convection zone into the overlying atmosphere is the driver of a diverse range of phenomena associated with solar activity. In this article, we introduce theoretical concepts central to the study of flux emergence and discuss how the inclusion of different phys...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Springer
2014-07-01
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| Series: | Living Reviews in Solar Physics |
| Subjects: | |
| Online Access: | http://www.livingreviews.org/lrsp-2014-3 |
| _version_ | 1797719518531813376 |
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| author | Mark C. M. Cheung Hiroaki Isobe |
| author_facet | Mark C. M. Cheung Hiroaki Isobe |
| author_sort | Mark C. M. Cheung |
| collection | DOAJ |
| description | Magnetic flux emergence from the solar convection zone into the overlying atmosphere is the driver of a diverse range of phenomena associated with solar activity. In this article, we introduce theoretical concepts central to the study of flux emergence and discuss how the inclusion of different physical effects (e.g., magnetic buoyancy, magnetoconvection, reconnection, magnetic twist, interaction with ambient field) in models impact the evolution of the emerging field and plasma. |
| first_indexed | 2024-03-12T09:07:04Z |
| format | Article |
| id | doaj.art-a0aa4b479d194ab1bbf7d2f8843b4566 |
| institution | Directory Open Access Journal |
| issn | 1614-4961 |
| language | English |
| last_indexed | 2024-03-12T09:07:04Z |
| publishDate | 2014-07-01 |
| publisher | Springer |
| record_format | Article |
| series | Living Reviews in Solar Physics |
| spelling | doaj.art-a0aa4b479d194ab1bbf7d2f8843b45662023-09-02T15:16:52ZengSpringerLiving Reviews in Solar Physics1614-49612014-07-0111310.12942/lrsp-2014-3lrsp-2014-3Flux Emergence (Theory)Mark C. M. Cheung0Hiroaki Isobe1Lockheed Martin Solar & Astrophysics Laboratory, 3251 Hanover St, Palo Alto, CA 94304, USAKwasan Observatory, Kyoto University, Yamashina, Kyoto 607-8471, JapanMagnetic flux emergence from the solar convection zone into the overlying atmosphere is the driver of a diverse range of phenomena associated with solar activity. In this article, we introduce theoretical concepts central to the study of flux emergence and discuss how the inclusion of different physical effects (e.g., magnetic buoyancy, magnetoconvection, reconnection, magnetic twist, interaction with ambient field) in models impact the evolution of the emerging field and plasma.http://www.livingreviews.org/lrsp-2014-3Radiative transferActive regionsMagnetohydrodynamics (MHD)Flux emergenceReconnectionConvectionPlasma physics |
| spellingShingle | Mark C. M. Cheung Hiroaki Isobe Flux Emergence (Theory) Living Reviews in Solar Physics Radiative transfer Active regions Magnetohydrodynamics (MHD) Flux emergence Reconnection Convection Plasma physics |
| title | Flux Emergence (Theory) |
| title_full | Flux Emergence (Theory) |
| title_fullStr | Flux Emergence (Theory) |
| title_full_unstemmed | Flux Emergence (Theory) |
| title_short | Flux Emergence (Theory) |
| title_sort | flux emergence theory |
| topic | Radiative transfer Active regions Magnetohydrodynamics (MHD) Flux emergence Reconnection Convection Plasma physics |
| url | http://www.livingreviews.org/lrsp-2014-3 |
| work_keys_str_mv | AT markcmcheung fluxemergencetheory AT hiroakiisobe fluxemergencetheory |