Coronal electron acceleration and relativistic proton production during the 14 July 2000 flare and CME

K.-L. Klein¹ - G. Trottet¹ - P. Lantos¹ - J.-P. Delaboudinière²

1 - DASOP, CNRS-UMR 8645, Observatoire de Paris, Section de Meudon, 92195 Meudon, France
2 - Institut d'Astrophysique Spatiale, Université Paris-Sud-CNRS, Bât. 121, 91405 Orsay, France

A&A 373, 1073-1082 (2001), DOI: 10.1051/0004-10361:20010653

In the radio spectrum of the 14 July 2000 event plotted in Fig. 2 the time axis of the IZMIRAN spectrum (25-100 MHz) contains an error. The corrected figure is reproduced here. The error does not affect the argumentation and conclusion of the paper.

$\begin{figure}\par\includegraphics[width=8.8cm,clip]{ms1241f2_corr.eps}\end{figure}$	Figure 2: Radio spectra from microwaves to hectometric waves during the 14 July 2000 event. From top to bottom: Ondrejov Observatory (Karlický et al. 2001), Artemis-IV, Thermopylae, Greece (courtesy C. Alissandrakis; Caroubalos et al. 2001), IZMIRAN, WAVES/Wind (courtesy M. Kaiser). Dark shading means bright emission.
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