Time-latitude prominences distribution (1967-2006)

Details Time-latitude prominences distribution (1967-2006) Time-latitude prominences distribution (1967-2006)

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007coska..37..184m&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 37, no. 3, p. 184-188.

Astronomy and Astrophysics

Astronomy

2

Sun: Activity, Sun: Magnetic Fields, Sun: Prominences

Scientific paper

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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