Method to determine the solar cycle length from the 530.3 nm green line corona

Details Method to determine the solar cycle length from the 530.3 nm green line corona Method to determine the solar cycle length from the 530.3 nm green line corona

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..133m&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 Cycles, Solar Activity

Scientific paper

The main periodicity in the solar activity is the 11-year cycle called the solar cycle. This period is not constant, but varies between of 9 and 14 years. The cycle length is conventionally defined as the time difference between two successive sunspot minima. Here, we propose a new method to define the solar cycle length from the time-latitudinal distribution of the 530.3 nm green coronal emission line observations. The time-latitudinal solar cycle length is defined as a difference between two successive splitting of primary pole ward branches from main equator ward branches.

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