Solar Rotation Determined from Thomas Harriot's Sunspot Observations of 1611 to 1613

Details Solar Rotation Determined from Thomas Harriot's Sunspot Observations of 1611 to 1613 Solar Rotation Determined from Thomas Harriot's Sunspot Observations of 1611 to 1613

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sci...202.1079h&link_type=abstract

Science, Volume 202, Issue 4372, pp. 1079-1081

Computer Science

3

Scientific paper

In 1612 the sun's mean sidereal rotation rate was only 13.3 degrees per
day based on a series of 199 unpublished drawings by Harriot. By
comparison with the rates in 1625 to 1626 and 1642 to 1644 it appears
that the solar rotation was accelerating significantly in the cycles
leading up to the Maunder minimum.

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