Journal
LIVING REVIEWS IN SOLAR PHYSICS
Volume 11, Issue 3, Pages 5-+Publisher
SPRINGER INTERNATIONAL PUBLISHING AG
DOI: 10.12942/lrsp-2014-3
Keywords
Flux emergence; Active regions; Magnetohydrodynamics (MHD); Plasma physics; Reconnection; Radiative transfer; Convection
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Funding
- International Space Science Institute in Bern, Switzerland
- NASA [NNX10AC02G, NNM07AA01C, NNX08BB02G]
- NASA [NNX08BB02G, 89964, NNX10AC02G, 135828] Funding Source: Federal RePORTER
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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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