The properties of solar radio spikes with harmonics and the associated EUV brightenings
Author:
- 4 January 2019
- journal article
- research article
- Published by Springer Nature in Astrophysics and Space Science
- Vol. 364 (1) , 4
Abstract
No abstract availableKeywords
This publication has 31 references indexed in Scilit:
- High resolution observations with Artemis-IV and the NRHAstronomy & Astrophysics, 2016
- A tiny event producing an interplanetary type III burstAstronomy & Astrophysics, 2015
- A UNIFIED COMPUTATIONAL MODEL FOR SOLAR AND STELLAR FLARESThe Astrophysical Journal, 2015
- Fine Structure of Metric Type IV Radio Bursts Observed with the ARTEMIS-IV Radio-Spectrograph: Association with Flares and Coronal Mass EjectionsSolar Physics, 2014
- Spiky Fine Structure of Type III-like Radio Bursts in AbsorptionSolar Physics, 2010
- Correlation between decimetric radio emission and hard X-rays in solar flaresAstronomy & Astrophysics, 2009
- Do solar decimetric spikes originate in coronal X-ray sources?Astronomy & Astrophysics, 2009
- Millisecond radio spikes in the decimetre band and their related active solar phenomenaAstronomy & Astrophysics, 2005
- Location of narrowband spikes in solar flaresAstronomy & Astrophysics, 2002
- Millisecond radio spikesSolar Physics, 1986