- Abstract:
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The Sun provides us with the only spatially well-resolved astrophysical example of turbulent thermal convection. While various aspects of solar photospheric turbulence, such as granulation (one-Megameter horizontal scale), are well understood, the questions of the physical origin and dynamical organization of larger-scale flows, such as the 30-Megameters supergranulation and flows deep in the solar convection zone, remain largely open in spite of their importance for solar dynamics and magnet...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 9.8mb)
-
- Publisher copy:
- 10.1051/0004-6361/201629747
-
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- Funding agency for:
- Schekochihin, AA
- Funding agency for:
- Schekochihin, AA
- Publisher:
- EDP Sciences Publisher's website
- Journal:
- Astronomy and Astrophysics Journal website
- Volume:
- 599
- Issue:
- March 2017
- Pages:
- Article: A69
- Publication date:
- 2017
- DOI:
- EISSN:
-
1432-0746
- ISSN:
-
0004-6361
- Pubs id:
-
pubs:646235
- URN:
-
uri:695e0d12-f6ff-4cc3-b62d-9859a514c50f
- UUID:
-
uuid:695e0d12-f6ff-4cc3-b62d-9859a514c50f
- Local pid:
- pubs:646235
- Copyright holder:
- ESO
- Copyright date:
- 2017
- Notes:
-
Copyright © 2017 ESO.
Journal article
Supergranulation and multiscale flows in the solar photosphere: Global observations vs. a theory of anisotropic turbulent convection
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