A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum (2008)
Attributed to:
Solar and Magnetospheric Plasma Theory
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361:20078834
Publication URI: http://dx.doi.org/10.1051/0004-6361:20078834
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics
Issue: 3