|
|
|
|
|||||||||||||||
|
|
|
|
|||||||||||||||
|
|||||||||||||||||
|
|||||||||||||||||
|
Record Search Query:
[Science_Parameters: Science_Category='EARTH SCIENCE', Science_Topic='SUN-EARTH INTERACTIONS', Science_Term='SOLAR ACTIVITY']
Potential Field Source Surface Models
Entry ID: PFSS
Summary
Abstract:
Potential Field Source Surface Models provide an approximate description of the solar coronal magnetic field based on observed photospheric fields (magnetograms). They were initially developed by Altschuler and Newkirk (Sol. Phys. 9, 131, 1969) and Schatten et al. (Sol. Phys. 6, 442, 1969), and later refined by Hoeksema (1984 Thesis, Stanford University) and Wang and Sheeley (ApJ 392, 310, 1992).
... ![]()
Related URL
Multimedia Sample
Service Citation
Service Keywords
Science Keywords
ISO Topic Category
Ancillary Keywords
Service Provider
Distribution Media
Personnel
Publications/References
Altschuler, M.D. and G. Newkirk, Magnetic fields and structure of solar corona .I. Methods of calculating coronal fields, Solar Physics 9, 131, 1969.
Hoeksema, J. T. 1984, Ph.D. thesis, Stanford University. Schatten, K. H., Wilcox J. M, and N. F. Ness, A model of interplanetary and coronal magnetic fields, Solar Physics, 6, 442, 1969. Wang, Y. M. And N. R. Sheeley , On potential-field models of the solar corona, Astrophysical Journal 392 (1): 310-319 Part 1 JUN 10 1992.
Creation and Review Dates
|
|||||||||||||||||
|
|
|||||||||||||||||
|
|
|
|
|||||||||||||||