期刊
LIVING REVIEWS IN SOLAR PHYSICS
卷 11, 期 3, 页码 5-+出版社
SPRINGER INTERNATIONAL PUBLISHING AG
DOI: 10.12942/lrsp-2014-3
关键词
Flux emergence; Active regions; Magnetohydrodynamics (MHD); Plasma physics; Reconnection; Radiative transfer; Convection
资金
- International Space Science Institute in Bern, Switzerland
- NASA [NNX10AC02G, NNM07AA01C, NNX08BB02G]
- NASA [NNX08BB02G, 89964, NNX10AC02G, 135828] Funding Source: Federal RePORTER
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.
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