group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
106 | 592 | 62 | 360 | 12.34 | 201.57 | -34.06 | 75.10 | 0.5643 | 167.1 | 54.7 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
3 | 33 | 2 | 18 | 9.31 | 212.14 | -23.49 | 77.89 | 0.4040 | 1172.6 | 902.1 | |
5 | -1 | 2 | -1 | 9.02 | 211.85 | -23.78 | 78.70 | 0.4078 | 1229.6 | 999999 | |
0 | 4 | 0 | 2 | 11.34 | 211.05 | -24.58 | 73.57 | 0.4270 | 848.0 | 713.4 | |
5 | 15 | 3 | 8 | 9.99 | 211.12 | -24.51 | 76.67 | 0.4216 | 1073.2 | 731.1 | |
0 | 5 | 0 | 3 | 12.09 | 210.84 | -24.79 | 71.97 | 0.4329 | 769.0 | 683.2 | |
0 | 7 | 0 | 4 | 11.65 | 210.80 | -24.83 | 72.99 | 0.4319 | 998.0 | 878.9 | |
0 | 10 | 0 | 6 | 10.29 | 210.48 | -25.15 | 76.25 | 0.4323 | 778.0 | 606.0 | |
0 | 4 | 0 | 2 | 11.26 | 209.72 | -25.91 | 74.41 | 0.4468 | 517.0 | 408.8 | |
0 | 4 | 0 | 2 | 8.54 | 209.46 | -26.17 | 80.54 | 0.4440 | -414.0 | -331.4 | |
6 | 14 | 3 | 8 | 11.04 | 209.20 | -26.43 | 75.11 | 0.4539 | 1029.1 | 807.6 | |
0 | 3 | 0 | 2 | 11.55 | 209.06 | -26.57 | 74.06 | 0.4576 | 575.0 | 575.6 | |
0 | 7 | 0 | 4 | 12.82 | 208.69 | -26.94 | 71.57 | 0.4675 | -508.0 | -403.6 | |
3 | 27 | 2 | 15 | 11.73 | 208.45 | -27.18 | 73.96 | 0.4672 | 951.3 | 784.3 | |
7 | 22 | 4 | 13 | 12.40 | 208.33 | -27.30 | 72.61 | 0.4713 | 1107.4 | 771.1 | |
4 | 36 | 2 | 20 | 11.01 | 208.48 | -27.15 | 75.46 | 0.4646 | 910.2 | 703.9 | |
2 | -15 | 1 | -15 | 11.24 | 208.23 | -27.40 | 75.08 | 0.4690 | 783.0 | 999999 | |
5 | -13 | 3 | -13 | 11.91 | 207.98 | -27.65 | 73.79 | 0.4749 | 936.5 | 999999 | |
0 | 5 | 0 | 3 | 8.93 | 208.17 | -27.46 | 80.01 | 0.4644 | -627.0 | -379.2 | |
5 | 18 | 3 | 10 | 12.64 | 207.34 | -28.29 | 72.57 | 0.4866 | 955.0 | 779.2 | |
0 | 4 | 0 | 2 | 9.77 | 207.19 | -28.44 | 78.50 | 0.4809 | 542.0 | 420.3 | |
0 | 6 | 0 | 4 | 11.59 | 206.86 | -28.76 | 74.90 | 0.4902 | 859.0 | 633.6 | |
6 | 15 | 3 | 9 | 13.10 | 205.79 | -29.83 | 72.35 | 0.5105 | 960.9 | 649.7 | |
0 | 5 | 0 | 3 | 12.21 | 205.54 | -30.09 | 74.17 | 0.5114 | 604.0 | 417.7 | |
0 | 6 | 0 | 3 | 10.19 | 204.93 | -30.70 | 78.26 | 0.5153 | 608.0 | 539.6 | |
0 | 3 | 0 | 2 | 12.52 | 204.27 | -31.36 | 74.05 | 0.5305 | 648.0 | 674.9 | |
18 | 68 | 10 | 40 | 12.29 | 203.68 | -31.95 | 74.67 | 0.5382 | 1228.5 | 463.5 | |
0 | 4 | 0 | 2 | 12.78 | 199.64 | -35.99 | 75.01 | 0.5955 | 461.0 | 339.2 | |
0 | 9 | 0 | 6 | 12.38 | 199.61 | -36.02 | 75.69 | 0.5950 | 561.0 | 453.2 | |
0 | 5 | 0 | 3 | 5.97 | 199.47 | -36.16 | 86.55 | 0.5901 | -315.0 | -319.0 | |
0 | 5 | 0 | 3 | 12.73 | 197.77 | -37.86 | 75.56 | 0.6204 | -823.0 | -732.4 | |
0 | 5 | 0 | 3 | 12.22 | 196.46 | -39.17 | 76.64 | 0.6368 | -755.0 | -702.7 | |
4 | 203 | 2 | 133 | 13.56 | 195.89 | -39.74 | 74.69 | 0.6466 | -1187.9 | -574.5 | |
0 | 12 | 0 | 8 | 11.31 | 195.88 | -39.75 | 78.16 | 0.6429 | -1191.0 | -896.5 | |
9 | -32 | 6 | -32 | 13.57 | 195.35 | -40.28 | 74.80 | 0.6535 | -1486.5 | 999999 | |
3 | -32 | 2 | -32 | 13.84 | 195.14 | -40.49 | 74.44 | 0.6568 | -1581.2 | 999999 | |
0 | 3 | 0 | 2 | 12.91 | 195.11 | -40.52 | 75.84 | 0.6554 | -565.0 | -484.8 | |
15 | -32 | 10 | -32 | 13.82 | 194.76 | -40.87 | 74.55 | 0.6615 | -1235.5 | 999999 | |
0 | 6 | 0 | 4 | 10.64 | 195.25 | -40.38 | 79.29 | 0.6503 | -867.0 | -726.8 | |
6 | -32 | 4 | -32 | 13.92 | 194.36 | -41.27 | 74.49 | 0.6667 | -750.6 | 999999 | |
0 | 6 | 0 | 4 | 13.11 | 193.55 | -42.08 | 75.85 | 0.6754 | -340.0 | -186.5 | |
0 | 3 | 0 | 2 | 10.58 | 193.54 | -42.09 | 79.59 | 0.6722 | -591.0 | -516.8 | |
0 | 6 | 0 | 4 | 13.70 | 192.59 | -43.04 | 75.16 | 0.6882 | -406.0 | -329.6 | |
0 | 4 | 0 | 3 | 12.10 | 192.77 | -42.86 | 77.45 | 0.6837 | -577.0 | -422.0 |
Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
B | - Heliographic latitude B; positive: North, negative: South | |
L | - Heliographic longitude L | |
LCM | - Longitudinal distance from the Sun's central meridian | |
Pos. angle | - Position angle | |
r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. |