Modeling the radial variation of coronal streamer belts during sunspot ascending phase

Modeling the radial variation of coronal streamer belts during sunspot ascending phase

The coronal streamer belts and their radial variation between 2.5 and 20.0 solar radii in the ascending phase of the solar cycle can be well reproduced using the horizontal current-current sheet-source surface magnetic field model with the set of model parameters determined based on MDI and LASCO Ca...

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Bibliographic Details
Published in:Advances in Space Research Vol. 29; no. 3; pp. 411 - 416
Main Authors: Zhao, X.P., Hoeksema, J.T., Rich, N.B.
Format: Journal Article Conference Proceeding
Language:English
Published: Elsevier Ltd 2002
Online Access:Get full text
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Summary:The coronal streamer belts and their radial variation between 2.5 and 20.0 solar radii in the ascending phase of the solar cycle can be well reproduced using the horizontal current-current sheet-source surface magnetic field model with the set of model parameters determined based on MDI and LASCO Carrington maps during 1996 minimum activity phase.
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ISSN:0273-1177
1879-1948
DOI:10.1016/S0273-1177(01)00604-4