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Comprehensive Radio Monitoring Website for Solar Events

Explore a new web platform dedicated to radio monitoring of solar activities like CMEs and electron beams, combining data from various spectrographs. Access radio spectrums, 2D movies, and more for deep analysis. Enhance your understanding of solar dynamics!

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Comprehensive Radio Monitoring Website for Solar Events

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  1. A new web site for radio monitoringM. Pick, M. Maksimovic, J. L. Bougeret, A. Lecacheux, R. Romagnan, A. Bouteille, K. SuedileLESIA, Observatoire de ParisC. Alissandrakis, X. Moussas (Greece) Why a web site for radio monitoring ? Main objectives -Radio associated with CMEs, onset, development -Electron beams from the low corona to the interplanetary medium Goal: one radio spectrum in combining data from different spectrographs (large freq. Range) -Nançay Radioheliograph - SECCHI CME summary (R. Howard, A. Vourlidas) -Link with S-Waves pages

  2. Web Page • 1D-images (EW and SN) 164 MHz • Composite spectrum 600 MHz-≤ 25 MHz • Artemis • Nançay DAM spectrographs • WAVES/WIND • 2D-movie • Cad 120s 6-8 hours • ZOOM Cad 10s /1hours • RAD2 16S • Includes CME timing • Link with S-Waves • Stereo measurements (Nançay) DAM RAD1 RAD2 DAM ART NRH

  3. October 28 2003

  4. Moreton waves

  5. Web page • http://secchirh.obspm.fr 19980502.mpg

  6. 19980502 NRH 10s

  7. 164 MHz • Electrons trace the expansion of • the arch system(~2500 km/sec) • Coronal wave develops along • flank of CME In lateral expansion

  8. October 28 2003

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