Dynamics of active longitudes as inferred from sunspot observations

Details Dynamics of active longitudes as inferred from sunspot observations Dynamics of active longitudes as inferred from sunspot observations

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..105i&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Physics

1

Solar Activity, Sunspots

Scientific paper

The data from the Greenwich Observatory for 1879-2002 (cycles 12-23) have been used to plot a time (years) vs. Carrington longitude diagram of distribution of the rotation-summed sunspot areas. Then, the active longitudes have been identified on these diagrams by intensive long-lived features (sunspot formation zones). The behaviour of the active longitudes (their location, shift, and intensity variations) has been analysed over the entire time interval under consideration.

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