Identification
Title
Large scale flows in the solar convection zone
Abstract
We discuss the current theoretical understanding of the large scale flows observed in the solar convection zone, namely the differential rotation and meridional circulation. Based on multi-D numerical simulations we describe which physical processes are at the origin of these large scale flows, how they are maintained and what sets their unique profiles. We also discuss how dynamo generated magnetic field may influence such a delicate dynamical balance and lead to a temporal modulation of the amplitude and profiles of the solar large scale flows.
Resource type
document
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code
http://n2t.net/ark:/85065/d7ms3ts1
codeSpace
Dataset language
eng
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geoscientificInformation
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title
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date type
publication
effective date
2016-01-01T00:00:00Z
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publication
effective date
2009-04-01T00:00:00Z
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An edited version of this paper was published by Springer. Copyright Springer Science+Business Media B.V. 2008.
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None
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contact position
OpenSky Support
organisation name
UCAR/NCAR - Library
full postal address
PO Box 3000
Boulder
80307-3000
email address
opensky@ucar.edu
web address
http://opensky.ucar.edu/
name:
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pointOfContact
Metadata on metadata
Metadata point of contact
contact position
OpenSky Support
organisation name
UCAR/NCAR - Library
full postal address
PO Box 3000
Boulder
80307-3000
email address
opensky@ucar.edu
web address
http://opensky.ucar.edu/
name:
homepage
responsible party role
pointOfContact
Metadata date
2023-08-18T18:57:24.724493
Metadata language
eng; USA