Solar Fields

Longcope, Dana W. Topological Methods for the Analysis of Solar Magnetic Fields. Living Reviews in Solar Physics. 2005, 2. doi:10.12942/lrsp-2005-7.  Hornig

Magnetic Fields in the Cosmos, 2007, Princeton University Press. ISBN 978-0691128412. Lerner, Louise. Eugene Parker, 'legendary figure' in solar science

Opportunities for the Diagnostics of Solar and Stellar Magnetic Fields. ASP Conference Proceedings. Magnetic Fields Across the Hertzsprung-Russell Diagram

models  R.C. Altrock. The Temperature of the Low Corona During Solar Cycles 21–23. Solar Physics. 2004, 224: 255. Bibcode:2004SoPh..224..255A. doi:10

像是一般的流體，有著極區轉得較慢，赤道轉得較快的較差自轉。內部的輻射層可能是化石恆星磁場（英语：Fossil stellar magnetic fields），表現出鋼體的性質。內部的旋轉速率大致等於中緯度的自轉速率，即慢速的極區和快速的赤道之間的旋轉速率。日震學的最近結果顯示，差旋層位於0