Determine the strength of the toroidal magnetic fields at the base of the
convection zone, and of the core fields.
Giant loops in the solar
atmosphere may trigger Sun's magnetic poles reversals.
Torquing Up the Interior
of the Sun (link to Imperial College)
Solar-Cycle Changes in SOI and GONG Data for 1996-7,
Anderson, E. R., R. Howe, and R. Komm
SOHO6/GONG98, 901, 1998,
NASA ADS Astronomy Abstract Service link
Page last revised July 2, 2003.