On the scaling of waiting-time distributions of the negative IMF B-z component (Articolo in rivista)

Type
Label
  • On the scaling of waiting-time distributions of the negative IMF B-z component (Articolo in rivista) (literal)
Anno
  • 2006-01-01T00:00:00+01:00 (literal)
Alternative label
  • D'Amicis, R; Bruno, R; Bavassano, B; Carbone, V; Sorriso-Valvo, L (2006)
    On the scaling of waiting-time distributions of the negative IMF B-z component
    in Annales geophysicae (1988)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • D'Amicis, R; Bruno, R; Bavassano, B; Carbone, V; Sorriso-Valvo, L (literal)
Pagina inizio
  • 2735 (literal)
Pagina fine
  • 2741 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 24 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • INAF, Ist Fis Spazio Interplanetario, I-00133 Rome, Italy; Univ Calabria, Dipartimento Fis, I-87036 Arcavacata Di Rende, CS, Italy; CNR, INFM, Liquid Crystal Lab, I-87030 Arcavacata Di Rende, CS, Italy (literal)
Titolo
  • On the scaling of waiting-time distributions of the negative IMF B-z component (literal)
Abstract
  • Statistics associated with the fluctuations in solar wind parameters show a remarkable dependence on the solar activity phase. In particular, we focus our attention on the waiting-time statistics governing the MHD fluctuations of the z-component of the interplanetary magnetic field, which are important within the framework of the Sun-Earth connections, and briefly discuss the preliminary results. Data from several spacecrafts, covering different phases of the solar cycle and different radial distances, are used. We found that propagating Alfvenic fluctuations and convected structures strongly influence the statistics which vary from quasi-Poissonian to power law. (literal)
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