| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.45 | 423.81 | 37.79 | 220.79 | 15.25 | 232.59 | -11.60 | 38.64 | 0.3078 | -589.8 | -275.3 | |
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back to the solar disc SDO HMI 2011-11-25 01:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.53 | 15.14 | 236.86 | -7.33 | 27.88 | 0.2646 | -861.0 | -725.2 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 13.77 | 236.81 | -7.38 | 30.76 | 0.2450 | -697.0 | -597.9 | |
| 0.00 | 2.57 | 0.00 | 1.31 | 13.41 | 236.27 | -7.92 | 33.38 | 0.2447 | 592.0 | 538.3 | |
| 7.11 | 18.24 | 3.64 | 9.34 | 13.65 | 235.61 | -8.57 | 34.92 | 0.2542 | -1132.0 | -773.8 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 16.54 | 235.34 | -8.85 | 29.88 | 0.2973 | 912.0 | 639.7 | |
| 0.00 | 0.77 | 0.00 | 0.39 | 13.28 | 234.92 | -9.27 | 37.90 | 0.2563 | -929.0 | -614.0 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 16.90 | 234.41 | -9.77 | 31.72 | 0.3103 | -1046.0 | -792.4 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 17.70 | 234.37 | -9.82 | 30.46 | 0.3219 | -739.0 | -679.7 | |
| 0.00 | 2.74 | 0.00 | 1.43 | 17.36 | 234.26 | -9.92 | 31.30 | 0.3180 | -862.0 | -692.0 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 17.60 | 234.19 | -10.00 | 31.08 | 0.3221 | -827.0 | -664.8 | |
| 0.00 | 2.65 | 0.00 | 1.36 | 12.85 | 234.35 | -9.84 | 40.63 | 0.2569 | -852.0 | -804.4 | |
| 47.44 | 294.76 | 24.52 | 152.31 | 15.00 | 234.23 | -9.96 | 35.90 | 0.2862 | -1448.7 | -444.2 | |
| 0.00 | 2.14 | 0.00 | 1.11 | 14.96 | 232.29 | -11.89 | 40.85 | 0.3057 | -1057.0 | -862.7 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 17.53 | 231.85 | -12.34 | 36.67 | 0.3427 | -753.0 | -628.1 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 17.38 | 231.76 | -12.42 | 37.14 | 0.3415 | -945.0 | -817.9 | |
| 0.00 | 1.46 | 0.00 | 0.76 | 14.75 | 231.93 | -12.26 | 42.17 | 0.3072 | -834.0 | -664.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 14.08 | 231.84 | -12.34 | 43.93 | 0.3002 | -764.0 | -565.5 | |
| 1.20 | 2.14 | 0.64 | 1.14 | 18.51 | 231.27 | -12.92 | 36.15 | 0.3610 | -795.5 | -869.4 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 16.09 | 231.28 | -12.90 | 40.71 | 0.3304 | -708.0 | -579.6 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 16.67 | 231.18 | -13.01 | 39.76 | 0.3386 | -764.0 | -608.1 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 16.08 | 231.09 | -13.09 | 41.12 | 0.3325 | -843.0 | -690.2 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 17.36 | 229.53 | -14.65 | 41.69 | 0.3646 | -787.0 | -458.6 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 18.83 | 228.34 | -15.85 | 41.14 | 0.3946 | -480.0 | -419.8 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 17.38 | 227.99 | -16.20 | 44.43 | 0.3820 | -1047.0 | -804.0 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 19.05 | 227.79 | -16.39 | 41.69 | 0.4028 | -729.0 | -630.6 | |
| 0.00 | 2.57 | 0.00 | 1.39 | 19.29 | 227.51 | -16.68 | 41.74 | 0.4087 | -686.0 | -589.2 | |
| 0.00 | 1.97 | 0.00 | 1.06 | 17.07 | 227.37 | -16.82 | 46.07 | 0.3857 | 897.0 | 650.3 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 16.94 | 227.03 | -17.16 | 46.88 | 0.3884 | 1035.0 | 810.8 | |
| 0.00 | 1.20 | 0.00 | 0.64 | 15.68 | 226.59 | -17.59 | 50.12 | 0.3809 | 882.0 | 780.4 | |
| 0.00 | 1.71 | 0.00 | 0.92 | 17.06 | 226.40 | -17.79 | 47.63 | 0.3971 | 862.0 | 571.8 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 15.71 | 226.40 | -17.79 | 50.36 | 0.3836 | 878.0 | 705.8 | |
| 4.28 | 4.97 | 2.30 | 2.67 | 15.65 | 226.11 | -18.08 | 50.92 | 0.3866 | 1082.7 | 938.4 | |
| 5.91 | 54.72 | 3.18 | 29.52 | 15.98 | 225.63 | -18.56 | 50.94 | 0.3958 | 1276.9 | 690.9 | |
| 0.00 | 4.97 | 0.00 | 2.69 | 16.62 | 225.50 | -18.69 | 49.83 | 0.4036 | 723.0 | 631.9 | |
| 6.51 | -33.00 | 3.51 | -33.00 | 15.86 | 225.25 | -18.94 | 51.73 | 0.3994 | 960.6 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 15.19 | 225.31 | -18.88 | 53.04 | 0.3924 | 675.0 | 528.4 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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 | |
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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. | |