Chromospheric and coronal magnetic fields

Eric Priest*

*Corresponding author for this work

Research output: Book/ReportBook


A summary is given of the main results that have been presented at the conference, together with comments on them and suggestions for future work. In particular, this covers the structure of the magnetic field (in the photosphere, chromosphere and corona) and the dynamics of the magnetic field (in coronal heating, prominences, emerging flux, eruptive instability and waves).

Original languageEnglish
Number of pages12
Publication statusPublished - 1 Dec 2005
EventInternational Scientific Conference on Chromospheric and Coronal Magnetic Fields - Katlenburg - Lindau, Germany
Duration: 30 Aug 20052 Sept 2005

Publication series

NameEuropean Space Agency, (Special Publication) ESA SP
PublisherEuropean Space Agency
ISSN (Print)0379-6566


Dive into the research topics of 'Chromospheric and coronal magnetic fields'. Together they form a unique fingerprint.

Cite this