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The Solar Wind as a Turbulence Laboratory
DOI: 10.12942/lrsp-2005-4 Bibcode: 2005LRSP....2....4B

Bruno, Roberto; Carbone, Vincenzo

In this review we will focus on a topic of fundamental importance for both plasma physics and astrophysics, namely the occurrence of large-amplitude low-frequency fluctuations of the fields that describe the plasma state. This subject will be treated within the context of the expanding solar wind and the most meaningful advances in this research f…

2005 Living Reviews in Solar Physics
Ulysses 476
Local Helioseismology
DOI: 10.12942/lrsp-2005-6 Bibcode: 2005LRSP....2....6G

Gizon, Laurent; Birch, Aaron C.

We review the current status of local helioseismology, covering both theoretical and observational results. After a brief introduction to solar oscillations and wave propagation through in-homogeneous media, we describe the main techniques of local helioseismology: Fourier-Hankel decomposition, ring-diagram analysis, time-distance helioseismology,…

2005 Living Reviews in Solar Physics
SOHO 202
Magnetic Fields in the Solar Convection Zone
DOI: 10.12942/lrsp-2004-1 Bibcode: 2004LRSP....1....1F

Fan, Yuhong

Recent studies of the dynamic evolution of magnetic flux tubes in the solar convection zone are reviewed with focus on emerging flux tubes responsible for the formation of solar active regions. The current prevailing picture is that active regions on the solar surface originate from strong toroidal magnetic fields generated by the solar dynamo mec…

2004 Living Reviews in Solar Physics
SOHO 74