The green corona data: 1947 - 1976, revisited.

Details The green corona data: 1947 - 1976, revisited. The green corona data: 1947 - 1976, revisited.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ncimc..20..923s&link_type=abstract

Nuovo Cimento C, Vol. 20C, N. 6, p. 923 - 931

Physics

8

Solar Corona: Solar Activity Cycles, Solar Corona: Line Intensities

Scientific paper

Re-examining a continuous monthly data set for the green-line corona brightness, covering February 1947 to September 1976, the authors have found that practically no delay exists between the trends of the green-line coronal intensity in the equatorial and middle-latitude belts at the beginning of solar activity cycle No. 20, while a previous cycle (No. 19) shows a sudden increase in the corona intensity brightness at middle latitudes followed by a delayed one at the equatorial belts, supporting recent findings on even-odd solar cycle differences observed in the half-yearly green corona database (1943 - 1993). The north-south asymmetry in the hemispheric solar activity is not involved in this phenomenon.

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