Long-term variability of solar magnetic-fields

Abstract

Studies of the variations of the solar magnetic field are reviewed. Consideration is given to the study of 600 Myr-old Australiain varve data showing the 22-yr magnetic cycle and variations with 300-400 yr periods (Williams, 1981 and Bracewell, 1985). Methods of interpreting the organization of large-scale solar field patterns are discussed. Other studies examined include the interpretation of modal structure in the photospheric field by Stenflo et al. (1988), and the study of Sheeley et al. (1987) showing that much of the large-scale surface pattern can be deduced from the measured emerging flux.