Abstract
In this paper we present a measure of the synodic solar rotation rate derived from an analysis of a Flamsteed drawing, corroborating the decrease of the solar rotation in the deep Maunder minimum (1666–1700).
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References
Abarbanell, C. and Wöhl, H.: 1981, Solar Phys. 70, 197.
Eddy, J. A., Gilman, P. A., and Trotter, D. E.: 1976, Solar Phys. 46, 3.
Flamsteed, J.: 1684, Phil. Trans. 14, 535.
Hoyt, D. V. and Schatten, K. H.: 1995a, Solar Phys. 160, 371.
Hoyt, D. V. and Schatten, K. H.: 1995b, Solar Phys. 160, 379.
Nesme-Ribes, E., Ferreira, E. N., and Mein, P.: 1993, Astron. Astrophys. 274, 563.
Ribes, J. C. and Nesme-Ribes, E.: 1993, Astron. Astrophys. 276, 549.
Ward, F.: 1966, Astrophys. J. 145, 416.
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Vaquero, J., Sánchez-bajo, F. & Gallego, M. A Measure of the Solar Rotation During the Maunder Minimum. Solar Physics 207, 219–222 (2002). https://doi.org/10.1023/A:1016262813525
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DOI: https://doi.org/10.1023/A:1016262813525