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Paper: How Different Was the Last Solar Minimum?
Volume: 462, Progress in Solar/Stellar Physics with Helio- and Asteroseismology
Page: 261
Authors: Basu, S.; Chaplin, W. J.; Elsworth, Y.; Broomhall, A.; Jarvis, E.
Abstract: The activity minimum between solar Cycles 23 and 24 has been exceptional in its quietness. It had the lowest sustained 10.7 cm flux since since observation of this proxy began in 1947. The internal dynamics of the Sun have been found to be very different for the minimum of Cycle 24 compared with that of Cycle 23. There have only been preliminary attempts to determine whether there were differences in the structure of the Sun during the Cycle 24 minimum compared with the Cycle 23 minimum. Early studies have shown differences between solar oscillation frequencies at the two minima. We expand the earlier study and use a hybrid forward-modelling and fitting method to determine whether the frequency differences imply differences in the structure of the Sun between the two minima.
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