Event calendar file
3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
Merida, Mexico
-
Regency (Hyatt)
SH.1.7
Waiting time distribution of emissions in complex Coronal Mass Ejections
Speakers
- Dr. Adolfo MENDEZ BERHONDO
Primary authors
- Dr. Adolfo MENDEZ BERHONDO (Institute of Geophysics and Astronomy)
Co-authors
- Dr. Ramon RODRIGUEZ TABOADA (Institute of Geophysics and Astronomy)
- Ms. Liliana ALFONSO LARRALDE (Institute of Geophysics and Astronomy)
Files
Abstract content
The waiting time distribution of emissions in Coronal Mass Ejections (CMEs) with several emissions is examined. We define the waiting time () as the time interval between the commencement of an emission and the commencement of the next emission considered as parts of a unique CME. The distribution seems to follow a power-law.Two classes of CMEs several emissions are considered: “close” and “separate” depending on angular distance between emissions.
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 1 (SH), pages 185-188
