Plasma properties in eruptive prominences

Labrosse, N. (2013) Plasma properties in eruptive prominences. Proceedings of the International Astronomical Union, 8(S300), pp. 79-84. (doi:10.1017/S1743921313010776)

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Publisher's URL: http://dx.doi.org/10.1017/S1743921313010776

Abstract

Prominence eruptions are one of the most spectacular manifestations of our Sun's activity. Yet there is still some mystery surrounding their relevant physical conditions. What are their plasma parameters? How different are they from those of quiescent prominences? How do they relate to those within coronal mass ejections? We briefly review some recent results in non-LTE radiative transfer modelling which contribute to our knowledge of the plasma properties in eruptive prominences. We discuss in particular how these results, combined with observational data analysis, can help us in determining the plasma parameters in eruptive prominences.

Item Type:Articles
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Labrosse, Dr Nicolas
Authors: Labrosse, N.
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Proceedings of the International Astronomical Union
Publisher:Cambridge University Press
ISSN:1743-9213
ISSN (Online):1743-9221
Copyright Holders:Copyright © 2013 Cambridge University Press
First Published:First published in Proceedings of the International Astronomical Union 8(S300):79-84
Publisher Policy:Reproduced in accordance with the copyright policy of the publisher.

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