SDO HMI 2011-11-13 05:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.04 | 248.83 | 18.20 | 129.12 | 9.62 | 55.99 | 15.81 | 294.55 | 0.2962 | -517.9 | -358.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.69 | 208.82 | 7.14 | 108.82 | 9.28 | 57.46 | 17.28 | 290.57 | 0.3145 | -1307.5 | -455.6 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 7.34 | 57.22 | 17.03 | 284.73 | 0.3018 | -805.0 | -674.2 | |
| 18.08 | -1.00 | 9.41 | -1.00 | 9.49 | 57.09 | 16.91 | 291.61 | 0.3100 | -1499.1 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 11.06 | 55.92 | 15.74 | 297.84 | 0.3024 | -896.0 | -681.0 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 11.90 | 55.94 | 15.76 | 300.27 | 0.3090 | -801.0 | -598.8 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 10.02 | 55.80 | 15.62 | 294.79 | 0.2934 | -941.0 | -733.3 | |
| 0.00 | 1.46 | 0.00 | 0.76 | 11.04 | 55.67 | 15.49 | 298.12 | 0.2985 | -744.0 | -600.2 | |
| 0.00 | 1.55 | 0.00 | 0.79 | 10.25 | 51.50 | 11.32 | 303.02 | 0.2315 | -890.0 | -673.4 | |
| 0.00 | 2.15 | 0.00 | 1.10 | 12.09 | 50.62 | 10.44 | 311.57 | 0.2379 | 888.0 | 741.6 | |
| 1.29 | 1.64 | 0.65 | 0.83 | 9.91 | 50.02 | 9.84 | 305.33 | 0.2073 | -919.7 | -874.0 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 9.76 | 49.96 | 9.77 | 304.91 | 0.2050 | -980.0 | -719.2 | |
| 0.00 | 1.55 | 0.00 | 0.78 | 9.73 | 49.65 | 9.47 | 305.63 | 0.2004 | -1066.0 | -847.0 | |
| 0.00 | 2.58 | 0.00 | 1.30 | 9.17 | 48.57 | 8.39 | 306.45 | 0.1799 | 889.0 | 807.0 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 13.37 | 48.69 | 8.51 | 321.16 | 0.2307 | 1005.0 | 844.8 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 9.80 | 48.58 | 8.40 | 309.15 | 0.1866 | -905.0 | -647.5 | |
| 0.00 | 1.55 | 0.00 | 0.78 | 10.22 | 48.53 | 8.35 | 311.05 | 0.1905 | -1057.0 | -874.5 | |
| 0.00 | 0.69 | 0.00 | 0.35 | 10.70 | 48.55 | 8.37 | 312.88 | 0.1960 | -999.0 | -779.4 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 10.79 | 47.36 | 7.18 | 317.57 | 0.1829 | 761.0 | 505.1 | |
| 0.00 | 1.29 | 0.00 | 0.65 | 11.33 | 47.25 | 7.07 | 319.96 | 0.1885 | 971.0 | 769.2 | |
| 1.98 | 2.67 | 1.00 | 1.34 | 11.00 | 47.09 | 6.91 | 319.43 | 0.1825 | 868.7 | 638.4 | |
| 0.00 | 0.86 | 0.00 | 0.43 | 10.23 | 46.71 | 6.53 | 318.05 | 0.1682 | 886.0 | 651.8 | |
| 0.00 | 3.01 | 0.00 | 1.51 | 9.69 | 46.31 | 6.13 | 317.60 | 0.1567 | 846.0 | 790.9 | |
| 0.00 | 0.95 | 0.00 | 0.48 | 11.10 | 46.03 | 5.85 | 324.36 | 0.1725 | 733.0 | 548.2 | |
| 0.00 | 1.89 | 0.00 | 0.95 | 10.71 | 45.81 | 5.63 | 324.02 | 0.1649 | 861.0 | 677.4 | |
| 0.00 | 1.46 | 0.00 | 0.73 | 10.41 | 45.74 | 5.56 | 323.23 | 0.1601 | 935.0 | 692.6 | |
| 0.00 | 1.29 | 0.00 | 0.65 | 10.86 | 45.63 | 5.45 | 325.43 | 0.1652 | 925.0 | 672.6 | |
| 0.00 | 1.46 | 0.00 | 0.75 | 17.61 | 45.58 | 5.40 | 340.33 | 0.2676 | 812.0 | 658.9 | |
| 0.00 | 1.21 | 0.00 | 0.61 | 13.33 | 44.89 | 4.71 | 335.82 | 0.1958 | 886.0 | 648.3 | |
| 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. | |