Coronal mass ejections detected in solar mean magnetic field

Details Coronal mass ejections detected in solar mean magnetic field Coronal mass ejections detected in solar mean magnetic field

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000georl..27.3141b&link_type=abstract

Geophysical Research Letters, Volume 27, Issue 19, p. 3141-3144

Astronomy and Astrophysics

Astrophysics

4

Solar Physics, Astrophysics, And Astronomy: Coronal Mass Ejections, And Astronomy: Magnetic Fields

Scientific paper

One minute resolution solar mean magnetic field sequences during 74 coronal mass ejection events are analyzed using wavelet transforms. A significant fraction of the resulting wavelet power spectra shows a characteristic peak at the time of the coronal mass ejection. With an average period of 13 minutes, the signature in the solar mean field is most likely the result of global waves triggered by the departing CME.

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