CAOSP abstracts, Volume: 37, No.: 3, year: 2007

Abstract: This paper presents a study of the solar prominences time-latitude distribution for the period 1967-2007. The different patterns of the prominences distribution and its evolution during solar cycle are reported. The evolution of the different prominences patterns is closely related to the time-latitude topology of the large-scale magnetic field.

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Last update: September 18, 2007