Open Access
| Issue |
J. Space Weather Space Clim.
Volume 2, 2012
Space Climate
|
|
|---|---|---|
| Article Number | A12 | |
| Number of page(s) | 6 | |
| DOI | https://doi.org/10.1051/swsc/2012012 | |
| Published online | 14 August 2012 | |
- Cameron, R., and M. Schüssler, Solar cycle prediction using precursors and flux transport models, ApJ, 659, 801–811, 2007. [NASA ADS] [CrossRef] [Google Scholar]
- Charbonneau, P., and M. Dikpati, Stochastic fluctuations in a Babcock-Leighton model of the solar cycle, Astrophys. J., 543, 1027–1043, 2000. [CrossRef] [Google Scholar]
- Chernosky, E.J., A relationship between the length and activity of sunspot cycles, Publ. Astron. Soc. Pac., 66 (392), 241–247, 1954. [CrossRef] [Google Scholar]
- Clette, F., D. Berghmans, P. Vanlommel, R.A.M. van der Linden, A. Koeckelenbergh, and L. Wauters, From the Wolf Number to the International Sunspot Index: 25 years of SIDC, Adv. Space Res., 40 (7), 919–928, 2007. [NASA ADS] [CrossRef] [Google Scholar]
- Dikpati, M., P.A. Gilman, and G. de Toma, The Waldmeier effect: An artifact of the definition of Wolf sunspot number? ApJ, 673, L99–L101, 2008. [NASA ADS] [CrossRef] [Google Scholar]
- Du, Z., and S. Du, The relationship between the amplitude and descending time of a solar activity cycle, Sol. Phys., 238 (2), 431–437, 2006. [NASA ADS] [CrossRef] [Google Scholar]
- Du, Z.-L., H.-N. Wang, and X.-T. He, The relation between the amplitude and the period of solar cycles, Chin. J. Astron. Astrophys., 6, 489–494, 2006. [CrossRef] [Google Scholar]
- Faria, H.H., E. Echer, N.R. Rigozo, L.E.A. Vieira, D.J.R. Nordemann, and A. Prestes, A comparison of the spectral characteristics of the Wolf Sunspot Number (RZ) and Group Sunspot Number (RG), Sol. Phys., 223 (1–2), 305–318, 2004. [NASA ADS] [CrossRef] [Google Scholar]
- Getko, R., The intermediate-term quasi-cycles of Wolf Number and Group Sunspot Number fluctuations, Sol. Phys., 238 (1), 187–206, 2006. [CrossRef] [Google Scholar]
- Hathaway, D.H., R.M. Wilson, and E.J. Reichmann, Group Sunspot Numbers: Sunspot cycle characteristics, Sol. Phys., 211 (1), 357–370, 2002. [Google Scholar]
- Hoyt, D.V., and K.H. Schatten, Sunspot numbers: A new solar activity reconstruction, Sol. Phys., 179 (1), 189–219, 1998. [NASA ADS] [CrossRef] [Google Scholar]
- Karak, B.B., and A.R. Choudhuri, The Waldmeier effect and the flux transport solar dynamo, MNRAS, 410, 1503–1512, 2011. [Google Scholar]
- Li, K.J., P.X. Gao, and T.W. Su, The Schwabe and Gleissberg Periods in the Wolf Sunspot Numbers and the Group Sunspot Numbers, Sol. Phys., 229 (1), 181–198, 2005. [CrossRef] [Google Scholar]
- Li, K.J., and H.F. Liang, Relationship between Group Sunspot Numbers and Wolf Sunspot Numbers, Astron. Nachr., 331 (7), 709–715, 2010. [CrossRef] [Google Scholar]
- Solanki, S.K., N.A. Krivova, M. Schüssler, and M. Fligge, Search for a relationship between solar cycle amplitude and length, Astron. Astrophys., 396, 1029–1035, 2002. [Google Scholar]
- Svalgaard, L., Updating the historical sunspot record, in SOHO-23: Understanding a Peculiar Solar Minimum, eds.S.R., Cranmer, J.T. Hoeksema, and J.L. KohlASP Conference Series, 428, 297–306, 2010. [Google Scholar]
- Vaquero, J.M., Historical sunspot observations: A review, Adv. Space Res., 40, 929–941, 2007. [Google Scholar]
- Vaquero, J.M., and R.M. Trigo, Can the solar cycle amplitude be predicted using the preceding solar cycle length? Sol. Phys., 250 (1), 199–206, 2008. [CrossRef] [Google Scholar]
- Waldmeier, M., Die Zonenwanderung der Sonnenflecken, Astron. Mitt. Zürich, 14, 470–481, 1939. [Google Scholar]
- Wilson, R.M., D.H. Hathaway, and E.J. Reichmann, An estimate for the size of cycle 23 based on near minimum conditions, J. Geophys. Res., 103 (A4), 6595–6603, 1998. [NASA ADS] [CrossRef] [Google Scholar]
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.