Prominences in SDO/EVE spectra: contributions from large solar structures

Labrosse, N. , Hudson, H. and Kazachenko, M. (2013) Prominences in SDO/EVE spectra: contributions from large solar structures. Proceedings of the International Astronomical Union, 8(S300), pp. 439-440. (doi:10.1017/S1743921313011459)

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Publisher's URL: http://dx.doi.org/10.1017/S1743921313011459

Abstract

The EVE instrument on SDO is making accurate measurements of the solar spectral irradiance in the EUV between 30 and 1069 Å, with 1 Å spectral resolution and 10 s sampling rate. These data define solar variability in the “Sun-as-a-star” mode and reveal many interesting kinds of variation. Its high sensitivity also makes it suitable for spectroscopic diagnostics of solar features such as flares. Here we present EVE's potential contribution to the diagnostics of large-scale, slowly evolving features such as prominences and active regions, and what we can learn from this.

Item Type:Articles
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Labrosse, Dr Nicolas and Hudson, Dr Hugh
Authors: Labrosse, N., Hudson, H., and Kazachenko, M.
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):439-440
Publisher Policy:Reproduced in accordance with the copyright policy of the publisher.

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