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J.R. Kuhn, J.D. Armstrong (Institute for Astronomy)
Solar luminosity and irradiance variations provide an important constraint on the physics of the solar cycle. Starting from magnetic flux-transport models of the solar cycle it is possible to reproduce many of the features of the magnetic, irradiance, and acoustic solar cycle observables. This talk will describe how a ``delayed oscillator" model could explain the magnetic cycle.
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Bulletin of the American Astronomical Society, 34
© 2002. The American Astronomical Soceity.