What's going on?


"The single, physically most important parameter to study in prominences may be the magnetic field. Shapes, motions, and in fact the very existence of prominences depend on the nature of the magnetic field threading the prominence plasma." (Einar Tandberg-Hanssen 1974)


List of publications

(updated November 28, 2005) ADS search: direct access


Reprints of these articles are available upon request. However, you may also get copies of them through the NASA Astrophysics Data System (CfA Harvard, USA) or at the ADS mirror site (CDS Strasbourg, France). Recent articles printed in Astronomy & Astrophysics are also available in the electronic edition.