Peculiar features in the solar coronal hole occurrence (Articolo in rivista)

Type
Label
  • Peculiar features in the solar coronal hole occurrence (Articolo in rivista) (literal)
Anno
  • 2002-01-01T00:00:00+01:00 (literal)
Alternative label
  • Hofer M.Y., Storini M. (2002)
    Peculiar features in the solar coronal hole occurrence
    in Solar physics
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • Hofer M.Y., Storini M. (literal)
Pagina inizio
  • 1 (literal)
Pagina fine
  • 10 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 207 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Titolo
  • Peculiar features in the solar coronal hole occurrence (literal)
Abstract
  • A good knowledge of coronal hole (CH) evolution in time is relevant for the understanding of the decay and/or the stability of large-scale magnetic fields in the different heliographic latitudinal belts. Using a CH catalogue, mainly compiled from the He I line (10830 Å) measurement (Sanchez-Ibarra and Barraza-Paredes, 1992, and updated from the NOAA/BoulderWeb pages), some characteristics of the CH behaviour in the solar activity cycles 21 and 22 are identified and described. We found: (i) the total number distributions for the isolated and polar coronal holes are similar, (ii) there is a north/south asymmetry, with a northern dominance in the number distribution of the polar coronal holes, (iii) a hint of a 22-year periodicity in the CH behaviour. In addition, two pairs of two isolated CHs with opposite polarity, maximum ages of more than 14 Carrington rotations, separated by about two years, are found during the early decreasing activity phase of each cycle. (literal)

Incoming links:


Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#rivistaDi
Prodotto
data.CNR.it