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)

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.