Kontar, E. P. and Nindos, A. (2018) Combined radio and space-based solar observations: from techniques to new results – preface. Solar Physics, 293(6), 90. (doi: 10.1007/s11207-018-1309-2)
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Abstract
The phenomena observed at the Sun have a variety of unique radio signatures that can be used to diagnose the processes in the solar atmosphere. The insights provided by radio observations are further enhanced when they are combined with observations from space-based telescopes. This Topical collection demonstrates the power of combination methodology at work and provides new results on i) type I solar radio bursts and thermal emission to study active regions; ii) type II and IV bursts to better understand the structure of coronal mass ejections; and iii) non-thermal gyro-synchrotron and/or type III bursts to improve the characterisation of particle acceleration in solar flares. The ongoing improvements in time, frequency, and spatial resolutions of ground-based telescopes reveal new levels in the complexity of solar phenomena and pose new questions.
| Item Type: | Articles (Editorial) |
|---|---|
| Status: | Published |
| Refereed: | Yes |
| Glasgow Author(s) Enlighten ID: | Kontar, Professor Eduard |
| Authors: | Kontar, E. P., and Nindos, A. |
| College/School: | College of Science and Engineering > School of Physics and Astronomy |
| Journal Name: | Solar Physics |
| Publisher: | Springer |
| ISSN: | 0038-0938 |
| ISSN (Online): | 1573-093X |
| Published Online: | 19 June 2018 |
| Copyright Holders: | Copyright © 2018 Springer Nature B.V. |
| First Published: | First published in Solar Physics 293(6): 90 |
| Publisher Policy: | Reproduced in accordance with the publisher copyright policy |
| Related URLs: |
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