Article contents
Boundary Fitting Problems Associated with Coronal Magnetic Models
Published online by Cambridge University Press: 25 May 2016
Abstract
The calculation of coronal magnetic fields was first suggested by Gold (1958). Altschuler and Newkirk (1969) and Newkirk et al. (1968) used a Legendre polynomial fit to the photospheric observations of magnetic fields whereas Schatten (1968) with Wilcox and Ness (Schatten et al., 1969) use a magnetic monopole fit, first incorporated by Schmidt (1964).
- Type
- Part I Magnetic Structure Responsible for Coronal Disturbances
- Information
- Copyright
- Copyright © Reidel 1974
References
- 1
- Cited by