Hemispheric sunspot numbers R~n and R~s from 1945-2004: catalogue and N-S asymmetry analysis for solar cycles 18-23
By M. Temmer, J. Rybák, P. Bendik, Astrid Veronig, F. L. Vogler, W. Otruba, W. Pötzi, A. Hanslmeier. 2006
174 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Oceanography
View Paper: https://www.semanticscholar.org/paper/829f427ed25e62deef5b58f9758c18ebd5f8274f
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In Oceanography
Citations in the corpus
- ON THE WEAKENING OF THE POLAR MAGNETIC FIELDS DURING SOLAR CYCLE 23 (2009, background): “We also note a general tendency for the south pole to have stronger average fields than the north pole; this asymmetry is consistent with sunspot activity being greater in the southern hemisphere during the declining phases of the last four cycles (Temmer et al. 2006).”
- From the Wolf number to the International Sunspot Index: 25 years of SIDC (2007, methodology): “Therefore, a significant effort has been undertaken by the Kanzelhö he Observatory (Temmer et al., 2006) to reconstruct the hemispheric sunspot numbers, but currently the reconstruction spans only 6 cycles, back to 1940 and with a 80% partial coverage using two stations (Kanzelhö he and Skalnaté Ple”