Dynamo Wave Propagation
Dynamo Wave Propagation is a theoretical construct in solar dynamo theory that describes the spatial and temporal evolution of magnetic field generation due to the interaction between turbulent convective flows and differential rotation in the Sun’s interior, distinguished by its wave-like behavior in latitude and depth arising from the combined effects of the α-effect and meridional circulation.
141
Publications
10.8K
Citations
232
Authors
143
Institutions
Publications per year
2017–2026
10
Parents
141
E. N. Parker · The Astrophysical Journal · 1955 · 2K citations
Natural Sciences, Astronomy, Physics +14
Astrophysical magnetic fields and nonlinear dynamo theory
Axel Brandenburg, Kandaswamy Subramanian · Physics Reports · 2005 · 1.7K citations · Full text
Mean-Field Magneto-hydrodynamics and Dynamo Theory
H. K. Moffatt · Planetary and Space Science · 1981 · 354 citations
1–5 of 141
232
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Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation, Russia
8 publications · 225 citations
8
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7
h-index
6
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5
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1–5 of 232
143

Lomonosov Moscow State University
Moscow, Russia
14 h-index
18 publications
493 citations
Max Planck Institute for Solar System Research
Göttingen, Germany
10 h-index
24 publications
1.3K citations

University of Exeter
Exeter, United Kingdom
8 h-index
15 publications
390 citations

NSF National Center for Atmospheric Research
Boulder, United States
6 h-index
9 publications
494 citations
NSF NCAR High Altitude Observatory
Boulder, United States
6 h-index
10 publications
685 citations

KTH Royal Institute of Technology
Stockholm, Sweden
6 h-index
13 publications
907 citations
University of Cambridge
Cambridge, United Kingdom
6 h-index
8 publications
397 citations

Stockholm University
Stockholm, Sweden
6 h-index
13 publications
907 citations
1–8 of 143
ApJ · 25 publications · 4.1K citations
18
h-index
13 publications · 430 citations
12
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9 publications · 321 citations
9
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7 publications · 289 citations
7
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6 publications · 227 citations
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