The solar benchmark: Rotational modulation of the Sun reconstructed from archival sunspot records
We use archival daily spot coverage measurements from Howard et al. to study the rotational modulation of the Sun as though it were a distant star. A quasi-periodic Gaussian process measures the solar rotation period P-rot = 26.3 +/- 0.1 d, and activity cycle period P-cyc = 10.7 +/- 0.3 yr. We attempt to search for evidence of differential rotation in variations of the apparent rotation period throughout the activity cycle and do not detect a clear signal of differential rotation, consistent with the null results of the hare-and-hounds exercise of Aigrain et al. The full reconstructed solar light curve is available online.
document
http://n2t.net/ark:/85065/d7tt4v0q
eng
geoscientificInformation
Text
publication
2016-01-01T00:00:00Z
publication
2019-01-18T00:00:00Z
Copyright 2019 Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society.
None
OpenSky Support
UCAR/NCAR - Library
PO Box 3000
Boulder
80307-3000
name: homepage
pointOfContact
OpenSky Support
UCAR/NCAR - Library
PO Box 3000
Boulder
80307-3000
name: homepage
pointOfContact
2023-08-18T19:17:59.755590