Table 1.
Hemispheric asymmetries for solar cycles 12–24.
Cycle | tmax | Max. | Max. | Max. | Rate | Rate | Rate | Cumul. | Cumul. | Predom. | Diff. | ΔtN | ΔtS | ΔtN − S |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
No. | ISN | N | S | ISN | N | S | N | S | Hem. | [%] | (mon) | (mon) | (mon) | |
12 | 12/1883 | 128 | 63 | 84 | 5.3 | 4.4 | 4.6 | 3258 | 4409 | South | 35.3 | −27 | −1 | −26 |
13 | 08/1893 | 148 | 64 | 97 | 7.1 | 5.6 | 5.3 | 4125 | 5090 | South | 23.4 | −13 | 0 | −13 |
14 | 10/1905 | 105 | 74 | 56 | 4.3 | 3.7 | 3.2 | 3778 | 3674 | North | 2.8 | 1 | 18 | −17 |
15 | 08/1917 | 184 | 102 | 79 | 13.6 | 6.6 | 7.4 | 4918 | 3920 | North | 25.5 | 0 | 1 | −1 |
16 | 06/1928 | 135 | 67 | 74 | 9.0 | 5.5 | 4.4 | 4391 | 3916 | North | 12.1 | 2 | −7 | 9 |
17 | 05/1937 | 199 | 128 | 106 | 9.3 | 8.3 | 5.8 | 6033 | 5996 | North | 0.6 | 2 | 14 | −12 |
18 | 06/1947 | 225 | 109 | 125 | 10.2 | 6.6 | 7.4 | 6658 | 6630 | North | 0.4 | 27 | −1 | 28 |
19 | 11/1957 | 293 | 168 | 141 | 13.6 | 8.6 | 9.1 | 9516 | 6741 | North | 41.2 | 17 | −6 | 23 |
20 | 02/1969 | 157 | 92 | 78 | 7.7 | 5.1 | 4.2 | 6732 | 5222 | North | 28.9 | 0 | 12 | −12 |
21 | 11/1979 | 235 | 126 | 122 | 9.0 | 7.0 | 7.1 | 6889 | 7146 | South | 3.7 | −2 | 5 | −7 |
22 | 09/1989 | 216 | 111 | 124 | 12.8 | 8.8 | 5.8 | 5839 | 6780 | South | 16.1 | −1 | 22 | −23 |
23 | 11/2001 | 184 | 92 | 98 | 8.0 | 4.6 | 4.7 | 5731 | 6514 | South | 13.7 | −16 | 4 | −20 |
24 | 03/2014 | 117 | 64 | 82 | 7.3 | 5.3 | 5.6 | 3412 | 3126 | North | 9.2 | −29 | −1 | −28 |
Notes. We list the cycle number, the time of the cycle maximum tmax in terms of the 13-month smoothed ISN, the amplitudes of the cycle maxima in the ISN as well as north and south HSN, the peak growth rate during the cycle rise phase (in units of month−1) for the ISN, north and south HSN, the cumulative sunspot numbers for the northern and southern hemispheres, the predominant hemisphere, the relative difference between the cumulative sunspot numbers of the two hemispheres, the time difference between the cycle maximum (ISN) and the north HSN (ΔtN) and the south HSN (ΔtS) as well as the time difference between the HSN maxima (ΔtN − S). For cycles where the difference between the cumulated HSN is < 1%, we give the predominant hemisphere in italics.
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