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Waiting Time Distribution of Emissions in Complex Coronal Mass Ejections

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Abstract

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.

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Authors and Affiliations

  1. Astronomy Department, Institute of Geophysics and Astronomy, Calle 212 No. 2906, La Coronela, La Lisa, La Habana, CP 11 600, Cuba

    Adolfo L. Méndez Berhondo, Ramón E. Rodríguez Taboada & Liliana Alfonso Larralde

Authors
  1. Adolfo L. Méndez Berhondo
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  2. Ramón E. Rodríguez Taboada
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  3. Liliana Alfonso Larralde
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Correspondence to Adolfo L. Méndez Berhondo.

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Berhondo, A.L.M., Taboada, R.E.R. & Larralde, L.A. Waiting Time Distribution of Emissions in Complex Coronal Mass Ejections. Astrophys Space Sci 302, 213–216 (2006). https://doi.org/10.1007/s10509-005-9036-1

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  • DOI: https://doi.org/10.1007/s10509-005-9036-1

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