Solar Cycle Variation of Real CME Latitudes

Details Solar Cycle Variation of Real CME Latitudes Solar Cycle Variation of Real CME Latitudes

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...667l.101s&link_type=abstract

The Astrophysical Journal, Volume 667, Issue 1, pp. L101-L104.

Astronomy and Astrophysics

Astronomy

4

Sun: Coronal Mass Ejections (Cmes)

Scientific paper

With the assumption of radial motion and uniform longitudinal distribution of coronal mass ejections (CMEs), we propose a method to eliminate projection effects from the apparent observed CME latitude distribution. This method has been applied to SOHO LASCO data from 1996 January to 2006 December. As a result, we find that the real CME latitude distribution had the following characteristics: (1) High-latitude CMEs (θ>60deg, where θ is the latitude) constituted 3% of all CMEs and mainly occurred during the time when the polar magnetic fields reversed sign. The latitudinal drift of the high-latitude CMEs was correlated with that of the heliospheric current sheet. (2) Four percent of all CMEs occurred in the range 45deg<=θ<=60deg. These midlatitude CMEs occurred primarily in 2000, near the middle of 2002, and in 2005, forming a prominent three-peak structure. (3) The highest occurrence probability of low-latitude (θ<45deg) CMEs was at the minimum and during the declining phase of the solar cycle. However, the highest occurrence rate of low-latitude CMEs was at the maximum and during the declining phase of the solar cycle. The latitudinal evolution of low-latitude CMEs did not follow the Spörer sunspot law, which suggests that many CMEs originated outside of active regions.

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