Titlebook: Secular Solar and Geomagnetic Variations in the Last 10,000 Years; F. R. Stephenson (Institute Director),A. W. Wolfen Book 1988 Kluwer Aca

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Secular Solar and Geomagnetic Variations in the Last 10,000 Years978-94-009-3011-7Series ISSN 1389-2185

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Analysis of Pre-Telescopic and Telescopic Sunspot Observationsth of the solar equator. A detailed catalogue of naked-eye sunspots from Far Eastern annals is compiled from both the pre-telescopic and telescopic periods. Analysis of these fragmentary records indicates a mean period of about 10 years.

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The Solar Diameter Since 1715all been disputed. If significant changes in the size of the Sun were established they would lead to variations in the gravitational potential energy on time scales shorter than evolutionary ones and substantial modifications would need to be made to our current understanding of the solar interior.

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Variability of the Present and Ancient Sun: A Test of Solar Uniformitarianismunspots and active regions) to years (the 11 and 22 yr cycles of sunspot and magnetic activity). Less certain in the available record of direct observations (now 378 years long) are solar changes of longer period, including a possible “Gleissberg” cycle of 80 to 90 yrs that is suggested in the envel

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The Sun Among the Stars: What Stars Indicate about Solar Variabilityfields. The stages of evolution of a one solar mass star are described, particularly with respect to the levels of magnetic activity that characterize those phases. Finally, we examine evidence for long-term variability in solar-like stars. In hyperactive cases, variability with time scales near 50