Changing magnetic fields in the solar interior

Baldner, C. S. ; Antia, H. M. ; Basu, S. ; Larson, T. P. (2009) Changing magnetic fields in the solar interior Astronomical Society of the Pacific Conference Series, 416 . pp. 289-292. ISSN 1050-3390

Full text not available from this repository.

Official URL:


Even-order a-coefficients show changes that are correlated with solar activity. We analyze Michelson Doppler Imager (MDI) data that are available for solar cycle 23 to try and determine the change in solar magnetic fields, particularly in the upper part of the convection zone. This is the region where the even-order a-coefficients show the largest change. We use a forward calculation to determine the change in the magnetic fields between the last solar minimum and solar maximum.

Item Type:Article
Source:Copyright of this article belongs to Astronomical Society of the Pacific.
ID Code:75699
Deposited On:24 Dec 2011 15:12
Last Modified:24 Dec 2011 15:12

Repository Staff Only: item control page