Highlights of Solar Radio Physics


January 16, 2015: Karl-Ludwig Klein and Sophie Masson Radio emission and relativistic proton acceleration in the large solar particle event of 20 Jan 2005


November 3, 2009: Hana Mészárosová, Marian Karlický, Ján Rybák, and Karel Jiricka Signatures of Magnetoacoustic Wave Trains in Solar Decimetric Radio Type IV Bursts

March 18, 2009: Monique Pick and Nicole Vilmer Sixty-five years of solar radioastronomy - review paper published


November 25, 2008: Ludwig Klein, Silja Pohjolainen and Lidia van Driel Gesztelyi Topical issue on solar radio physics published

October 2, 2008: Silja Pohjolainen, Jens Pomoell and Rami Vainio Fragmented radio emission reveals a shock passing through solar active region loops

August 21, 2008: Karl-Ludwig Klein Type III bursts, magnetic field extrapolations, and the propagation of solar energetic particles


December 27, 2007: Tim Bastian Synchrotron Radio Emission from a Fast Halo Coronal Mass Ejection

November 22, 2007: Nat Gopalswamy A New Wind/WAVES Type II Burst Catalog Available Online

April 24, 2007: Monique Pick Radio monitoring of solar activity

March 12, 2007: Karl-Ludwig Klein A solar type N burst at decametric wavelengths

February 7, 2007: Nat Gopalswamy Radio-quiet Fast and Wide Coronal Mass Ejections

January 4, 2007: Arnold Benz Are there Radio-quiet Solar Flares?

Earlier Highlights

An email notice of a new Highlight is posted to the CESRA email list, you can subscribe to these messages by sending an email to Silja at

How to submit a highlight:

If you do not know how to write HTML code, just send an email with the text, images and movies you wish to show. Links related to the text are always welcome! We will then edit and HTMLify it according to the 'highlight' format, and you can do a final check before it goes public.

If you do know some HTML and would like to see the page more or less as it will appear: first save the form of a previous highlight with the "view - page source" menu item on your browser and then edit your own text and image file names into it (it is best to have all files in a separate directory). You will see what it looks like with the "open file" command. Then send us the lot in an email.

Note: We prefer to receive plain text or clear self-made HTML code as it is very time-consuming to edit pages created with some conversion programs. Image files should be in a web readable format (.png, .jpg, or .gif).

Highlight material and requests should be sent to Silja Pohjolainen at

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