{ "id": "0912.3782", "version": "v10", "published": "2009-12-18T20:04:09.000Z", "updated": "2010-10-20T09:26:02.000Z", "title": "Radio Observations of the January 20, 2005 X-Class Event", "authors": [ "C. Bouratzis", "P. Preka-Papadema", "A. Hillaris", "P. Tsitsipis", "A. Kontogeorgos", "V. G. Kurt X. Moussas" ], "comment": "Accepted for publication in Solar Physics", "doi": "10.1007/s11207-010-9648-7", "categories": [ "astro-ph.SR" ], "abstract": "We present a multi-frequency and multi-instrument study of the 20 January 2005 event. We focus mainly on the complex radio signatures and their association with the active phenomena taking place: flares, CMEs, particle acceleration and magnetic restructuring. As a variety of energetic particle accelerators and sources of radio bursts are present, in the flare-ejecta combination, we investigate their relative importance in the progress of this event. The dynamic spectra of {Artemis-IV-Wind/Waves-Hiras with 2000 MHz-20 kHz frequency coverage, were used to track the evolution of the event from the low corona to the interplanetary space; these were supplemented with SXR, HXR and gamma-ray recordings. The observations were compared with the expected radio signatures and energetic-particle populations envisaged by the {Standard Flare--CME model and the reconnection outflow termination shock model. A proper combination of these mechanisms seems to provide an adequate model for the interpretation of the observational data.", "revisions": [ { "version": "v10", "updated": "2010-10-20T09:26:02.000Z" } ], "analyses": { "keywords": [ "radio observations", "x-class event", "reconnection outflow termination shock model", "energetic particle accelerators", "standard flare-cme model" ], "tags": [ "journal article" ], "publication": { "journal": "Solar Physics", "year": 2010, "month": "Dec", "volume": 267, "number": 2, "pages": 343 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 840668, "adsabs": "2010SoPh..267..343B" } } }