SDO HMI 2011-11-24 22:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.17 | 319.35 | 25.60 | 163.22 | 14.45 | 251.60 | 5.76 | 335.86 | 0.2470 | -466.9 | -331.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.20 | 0.00 | 0.63 | 18.38 | 258.14 | 12.30 | 324.89 | 0.3530 | -862.0 | -658.6 | |
| 0.00 | 4.79 | 0.00 | 2.53 | 18.11 | 257.29 | 11.45 | 326.29 | 0.3415 | -814.0 | -742.5 | |
| 42.21 | 276.79 | 21.54 | 141.22 | 13.97 | 252.48 | 6.64 | 332.16 | 0.2415 | -1378.7 | -473.0 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 16.62 | 252.35 | 6.51 | 337.12 | 0.2808 | -695.0 | -512.4 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 16.87 | 252.14 | 6.30 | 338.12 | 0.2832 | -813.0 | -569.9 | |
| 2.31 | -3.00 | 1.18 | -3.00 | 13.67 | 252.01 | 6.18 | 333.25 | 0.2333 | -1338.6 | 999999 | |
| 5.65 | -3.00 | 2.88 | -3.00 | 13.89 | 251.84 | 6.00 | 334.33 | 0.2352 | -1178.2 | 999999 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 12.35 | 250.10 | 4.26 | 338.56 | 0.1993 | 813.0 | 659.4 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 17.09 | 246.60 | 0.76 | 357.27 | 0.2668 | 908.0 | 674.9 | |
| 0.00 | 5.39 | 0.00 | 2.76 | 16.45 | 246.16 | 0.32 | 358.78 | 0.2556 | 408.0 | 865.1 | |
| 0.00 | 2.14 | 0.00 | 1.10 | 16.82 | 246.10 | 0.26 | 359.04 | 0.2618 | 1140.0 | 966.9 | |
| 0.00 | 1.80 | 0.00 | 0.92 | 17.40 | 245.42 | -0.42 | 1.48 | 0.2717 | 737.0 | 656.5 | |
| 0.00 | 1.88 | 0.00 | 0.97 | 17.31 | 245.23 | -0.60 | 2.15 | 0.2703 | 1074.0 | 866.6 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 17.31 | 244.43 | -1.41 | 4.99 | 0.2711 | 704.0 | 652.7 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 18.85 | 244.23 | -1.61 | 5.16 | 0.2972 | 733.0 | 582.4 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 18.08 | 244.20 | -1.63 | 5.50 | 0.2844 | 776.0 | 619.9 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 18.42 | 243.92 | -1.92 | 6.30 | 0.2905 | 760.0 | 767.0 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 19.35 | 243.78 | -2.05 | 6.37 | 0.3062 | 713.0 | 561.3 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.73 | 243.48 | -2.36 | 7.59 | 0.2965 | 961.0 | 819.3 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 19.16 | 243.25 | -2.58 | 8.09 | 0.3042 | 807.0 | 670.1 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 19.10 | 242.69 | -3.15 | 9.85 | 0.3047 | 837.0 | 667.0 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 18.66 | 242.42 | -3.42 | 10.97 | 0.2984 | 861.0 | 712.2 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.20 | 242.33 | -3.51 | 11.57 | 0.2910 | 929.0 | 679.6 | |
| 0.00 | 2.14 | 0.00 | 1.11 | 18.79 | 242.16 | -3.67 | 11.67 | 0.3012 | 724.0 | 626.4 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.41 | 242.11 | -3.73 | 12.11 | 0.2953 | 764.0 | 599.9 | |
| 0.00 | 1.97 | 0.00 | 1.02 | 18.04 | 239.62 | -6.22 | 20.11 | 0.3009 | 927.0 | 690.3 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 18.96 | 238.10 | -7.73 | 23.21 | 0.3244 | -879.0 | -754.1 | |
| 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. | |