Abstract
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 language | English |
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Number of pages | 12 |
Edition | 596 |
Publication status | Published - 1 Dec 2005 |
Event | International Scientific Conference on Chromospheric and Coronal Magnetic Fields - Katlenburg - Lindau, Germany Duration: 30 Aug 2005 → 2 Sept 2005 |
Publication series
Name | European Space Agency, (Special Publication) ESA SP |
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Publisher | European Space Agency |
ISSN (Print) | 0379-6566 |