1 |
Mursula K, Ulich Th, A New Method to Determine the Solar Cycle Length, Geophys. Res. Lett., 25, 1837-1840 (1998).
DOI
ScienceOn
|
2 |
Oh SJ, Chang HY, Change of Sunspot Groups Observed from 2002 to 2011 at ButterStar Observatory, JASS, 29, 245-251 (2012). http://dx.doi.org/10.5140/JASS.2012.29.3.245
과학기술학회마을
DOI
ScienceOn
|
3 |
Pesnell WD, Solar Cycle Predictions, Sol. Phys., 281, 507-532 (2012).
|
4 |
Petrovay K, Solar Cycle Prediction, LRSP, 7, 6-64 (2010).
|
5 |
Solanki SK, Krivova NA, Schussler M, Fligge M, Search for a Relationship between Solar Cycle Amplitude and Length, A&A, 396, 1029-1035 (2002).
DOI
ScienceOn
|
6 |
Tlatov AG, The Minimum Activity Epoch as a Precursor of the Solar Activity, Sol. Phys., 260, 465-477 (2009).
DOI
|
7 |
Usoskin IG, Mursula K, Kovaltsov GA, Cyclic Behaviour of Sunspot Activity during the Maunder Minimum, A&A, 354, L33-L36 (2000).
|
8 |
Usoskin IG, Mursula K, Kovaltsov GA, Heliospheric modulation of cosmic rays and solar activity during the Maunder minimum, JGR, 106, 16039-16046 (2001). http://dx.doi.org/10.1029/2000JA000105
DOI
|
9 |
Usoskin IG, Mursula K, Kovaltsov GA, An Upper Limit on Sunspot Activity During the Maunder Minimum, Sol. Phys., 224, 95-101 (2004).
DOI
|
10 |
Vaquero JM, Historical Sunspot Observations: A Review, AdSpR, 40, 929-941 (2007).
|
11 |
Vaquero JM, Trigo RM, Can the Solar Cycle Amplitude Be Predicted Using the Preceding Solar Cycle Length?, Sol. Phys., 250, 199-206 (2008).
DOI
|
12 |
Vaquero JM, Trigo RM, Gallego MC, A Simple Method to Check the Reliability of Annual Sunspot Number in the Historical Period 1610- 847, Sol. Phys., 277, 389-395 (2012).
DOI
|
13 |
Chang HY, Oh SJ, Does Correction Factor Vary with Solar Cycle?, JASS, 29, 97-101 (2012). http://dx.doi.org/10.5140/JASS.2012.29.2.097
과학기술학회마을
DOI
ScienceOn
|
14 |
Cho IH, Chang HY, Latitudinal Distribution of Sunspots Revisited, JASS, 28, 1-7 (2011). http://dx.doi.org/10.5140/JASS.2011.28.1.001
과학기술학회마을
DOI
ScienceOn
|
15 |
Harvey KL, White OR, What is Solar Cycle Minimum?, JGR, 104, 19759-19764 (1999). http://dx.doi.org/10.1029/1999JA900211
DOI
|
16 |
Dikpati M, Gilman PA, de Toma G, The Waldmeier Effect: An Artifact of the Definition of Wolf Sunspot Number?, ApJ, 673, L99-L101 (2008). http://dx.doi.org/10.1086/527360
DOI
|
17 |
Du ZL, Relationship Between Solar Maximum Amplitude and Max-Max Cycle Length, AJ, 132, 1485-1489 (2006).
DOI
ScienceOn
|
18 |
Hamid R, Galal A, Preliminary Prediction of the Strength of the 24th 11-year Solar Cycle. In: Bothmer, V, Hady, AA (eds.) Solar Activity and Its Magnetic Origin, Proc. IAU Symp. 233, Cambridge Univ. Press, Cambridge, 413-416 (2006).
|
19 |
Hathaway DH, Wilson RM, Reichmann, EJ, The Shape of the Sunspot Cycle, Sol. Phys., 151, 177-190 (1994).
DOI
|
20 |
Hoyt DV, Schatten KH, Group Sunspot Numbers: A New Solar Activity Reconstruction, Sol. Phys., 179, 189-219 (1998).
DOI
|
21 |
Javaraiah, J, Predicting the Amplitude of a Solar Cycle Using the North-South Asymmetry in the Previous Cycle: II. An improved Prediction for Solar Cycle 24, Sol. Phys., 252, 419-439 (2008).
DOI
|
22 |
Kane RP, Solar Cycle Predictions Based on Extrapolation of Spectral Components: An update, Sol. Phys., 243, 205-217 (2007).
DOI
|
23 |
Kim BY, Chang HY, Alternating Sunspot Area and Hilbert Transform Analysis, JASS, 28, 261-265 (2011). http://dx.doi.org/10.5140/JASS.2011.28.4.261
과학기술학회마을
DOI
ScienceOn
|
24 |
Brown GM, What Determines Sunspot Maximum, MNRAS, 174, 185-189 (1976).
DOI
|
25 |
Berghmans D, van der Linden RAM, Vanlommel P, Warnant R, Zhukov A, et al., Solar Activity: Nowcasting and Forecasting at the SIDC, AnGeo, 23, 3115-3128 (2005).
|