The Maunder minimum: North-south asymmetry in sunspot formation, mean sunspot latitudes, and the butterfly diagram

Details The Maunder minimum: North-south asymmetry in sunspot formation, mean sunspot latitudes, and the butterfly diagram The Maunder minimum: North-south asymmetry in sunspot formation, mean sunspot latitudes, and the butterfly diagram

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010arep...54..476n&link_type=abstract

Astronomy Reports, Volume 54, Issue 5, pp.476-480

Astronomy and Astrophysics

Astronomy

1

Scientific paper

An approach to reconstructing solar activity in the past is used to study its time evolution. It is already possible to reconstruct not only the general level of solar activity on long timescales, but also particular aspects of its development: sunspot dominance in either hemisphere, the drift and latitude spread of the sunspot-formation zone, and features in the spatial distribution of the activity at specific epochs, such as the Maunder minimum.

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