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Theoretical predictions of latitude dependencies in the solar windResults are presented which were obtained with the Winge-Coleman model for theoretical predictions of latitudinal dependencies in the solar wind. A first-order expansion is described which allows analysis of first-order latitudinal variations in the coronal boundary conditions and results in a second-order partial differential equation for the perturbation stream function. Latitudinal dependencies are analytically separated out in the form of Legendre polynomials and their derivative, and are reduced to the solution of radial differential equations. This analysis is shown to supply an estimate of how large the coronal variation in latitude must be to produce an 11 km/sec/deg gradient in the radial velocity of the solar wind, assuming steady-state processes.
Document ID
19750043959
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Winge, C. R., Jr.
Coleman, P. J., Jr.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1974
Subject Category
Solar Physics
Meeting Information
Meeting: Solar wind three; Third Conference
Location: Pacific Grove, CA
Start Date: March 25, 1974
End Date: March 29, 1974
Accession Number
75A28031
Funding Number(s)
CONTRACT_GRANT: NAS2-7251
Distribution Limits
Public
Copyright
Other

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