A comparison of differential rotation measurements – (Invited Review)
By J. Beck. 2000
189 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/a9554f638c13dbcea9a3a994eb7078ad4d46e0b1
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In Astronomy and Astrophysics
- Mark S. Miesch
- J. Toomre
- R. Howe
- Paul Charbonneau
- A. Brun
- J. Christensen-Dalsgaard
- M. Thompson
- S. Christe
In Molecular Biology
- Mark S. Miesch
- J. Toomre
- R. Howe
- J. Christensen-Dalsgaard
- M. Thompson
- Bernhard Fleck
- R. Marsden
- Monica G. Bobra
Citations in the corpus
- Solar Orbiter (2012, background): “However, because of the lack of out-of-the ecliptic observations, the nearpolar flow fields remain poorly mapped, as does the differential rotation at high latitudes (see Beck, 2000; Thompson et al., 2003 and Figure 17).”
- Magnetic Flux Transport at the Solar Surface (2014, unknown): “See also Beck (2000) for a review.”
- The SunPy Project: Open Source Development and Status of the Version 1.0 Core Package (2020, background): “When analyzing the dynamics of features on the solar disk, it is important to account for variations due to the apparent rotation of the Sun, which includes solar differential rotation, a latitudinally varying rotation rate due to the nonrigidity of the solar interior (see Beck 2000).”
- The Internal Rotation of the Sun (2003, methodology): “…tracking sunspots,dot-dashed linefrom magnetogram correlation tracking), and tracking Doppler features resulting from large-scale (supergranular) convective flow patterns (dotted line); the curves correspond to fits of the form given in Equation 1, with coefficients adapted from Beck (2000).”
- The Solar Orbiter mission (2020, background): “However, as described above the near-polar flow fields and the differential rotation at high latitudes (Beck 2000; Thompson et al. 2003) cannot be mapped well from locations near the ecliptic plane.”
- Solar Interior Rotation and its Variation (2009, background): “For an overview of such measurements, see Beck (2000). The usual explanation for the discrepancy is that while the Doppler techniques measure the velocity at the surface, the tracers such as sunspots are anchored in a faster-rotating layer deeper down. For example, Gilman and Foukal (1979) noted tha”