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March 23, 2015Astronomy and AstrophysicsOpen Access

Grand solar minima and maxima deduced from¹⁰Be and¹⁴C: magnetic dynamo configuration and polarity reversal

Fadil Inceoglu R. Simoniello Mads Faurschou Knudsen C. Karoff Jesper Olsen S. Turck‐Chièze Bo Holm Jacobsen

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Abstract

Aims. This study aims to improve our understanding of the occurrence and origin of grand solar maxima and minima.

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Cite This Study

Inceoglu et al. (2015) studied this question.

synapsesocial.com/papers/6a10d228cfa01e990d9f9b89 https://doi.org/10.1051/0004-6361/201424212

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Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

1For how long will the current grand maximum of solar activity persist?Original Research · 2008 · 122 citations
2Stochastic theory of minimal realizationOriginal Research · 1974 · 429 citations
3Atmospheric impact on beryllium isotopes as solar activity proxyOriginal Research · 2008 · 60 citations
4Chromospheric variations in main-sequence starsOriginal Research · 1995 · 1,055 citations
5A 600‐year annual 10Be record from the NGRIP ice core, GreenlandOriginal Research · 2009 · 188 citations

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