Three-dimensional stability of the solar tachocline
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20052928/pdf
Reference8 articles.
1. Stability of the Solar Latitudinal Differential Rotation Inferred from Helioseismic Data
2. Helioseismic Constraints on the Structure of the Solar Tachocline
3. Analysis of Hydrodynamic Stability of Solar Tachocline Latitudinal Differential Rotation using a Shallow‐Water Model
4. A spectral solution of the magneto-convection equations in spherical geometry
5. A Comparison of Solarp‐Mode Parameters from the Michelson Doppler Imager and the Global Oscillation Network Group: Splitting Coefficients and Rotation Inversions
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2. Phase Speed of Magnetized Rossby Waves that Cause Solar Seasons;The Astrophysical Journal;2018-08-02
3. Role of Interaction between Magnetic Rossby Waves and Tachocline Differential Rotation in Producing Solar Seasons;The Astrophysical Journal;2018-02-01
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