SDO HMI 2011-11-10 18:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.27 | 438.85 | 40.09 | 225.59 | 16.50 | 64.53 | -8.07 | 30.05 | 0.2660 | -727.6 | -426.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.45 | 20.67 | 71.05 | -1.55 | 4.87 | 0.2993 | -853.0 | -641.1 | |
| 0.00 | 2.84 | 0.00 | 1.45 | 16.72 | 69.79 | -2.81 | 11.52 | 0.2365 | -754.0 | -699.5 | |
| 0.00 | 1.21 | 0.00 | 0.61 | 16.42 | 69.64 | -2.96 | 12.41 | 0.2319 | -899.0 | -711.4 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 18.29 | 65.40 | -7.20 | 24.79 | 0.2850 | -849.0 | -595.8 | |
| 66.47 | 369.11 | 34.01 | 188.83 | 16.00 | 65.27 | -7.33 | 29.27 | 0.2519 | -1398.0 | -490.6 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 19.80 | 65.08 | -7.52 | 23.52 | 0.3100 | -822.0 | -676.3 | |
| 0.00 | 1.55 | 0.00 | 0.80 | 18.17 | 64.97 | -7.63 | 26.29 | 0.2863 | -887.0 | -686.9 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 19.80 | 64.86 | -7.74 | 24.13 | 0.3114 | -861.0 | -698.6 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 17.37 | 64.94 | -7.66 | 27.74 | 0.2747 | -701.0 | -518.2 | |
| 1.38 | 16.27 | 0.71 | 8.39 | 17.28 | 64.72 | -7.88 | 28.56 | 0.2750 | -810.5 | -678.2 | |
| 1.72 | -5.00 | 0.88 | -5.00 | 16.42 | 64.63 | -7.97 | 30.47 | 0.2634 | -855.5 | 999999 | |
| 4.74 | -5.00 | 2.43 | -5.00 | 16.15 | 64.52 | -8.08 | 31.39 | 0.2604 | -898.9 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 18.10 | 64.28 | -8.33 | 28.41 | 0.2906 | -683.0 | -542.9 | |
| 0.00 | 1.55 | 0.00 | 0.79 | 15.35 | 64.21 | -8.39 | 34.10 | 0.2522 | 48.0 | 75.3 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 18.90 | 63.82 | -8.78 | 28.32 | 0.3057 | -701.0 | -532.2 | |
| 3.27 | 4.05 | 1.68 | 2.08 | 16.54 | 63.81 | -8.79 | 32.70 | 0.2723 | -841.6 | -676.9 | |
| 0.00 | 3.79 | 0.00 | 1.96 | 18.00 | 63.46 | -9.14 | 30.85 | 0.2959 | -712.0 | -522.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 18.09 | 63.30 | -9.30 | 31.13 | 0.2986 | -672.0 | -549.4 | |
| 0.00 | 0.77 | 0.00 | 0.42 | 23.47 | 62.33 | -10.27 | 25.42 | 0.3826 | -736.0 | -585.4 | |
| 0.00 | 1.29 | 0.00 | 0.70 | 23.61 | 58.64 | -13.96 | 32.48 | 0.4134 | -959.0 | -777.4 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 18.34 | 58.40 | -14.20 | 41.89 | 0.3504 | 906.0 | 727.3 | |
| 0.00 | 2.50 | 0.00 | 1.33 | 19.75 | 57.72 | -14.88 | 40.45 | 0.3742 | 971.0 | 744.1 | |
| 0.00 | 1.46 | 0.00 | 0.77 | 18.15 | 57.83 | -14.77 | 43.35 | 0.3544 | 644.0 | 650.7 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 20.18 | 57.19 | -15.42 | 40.63 | 0.3848 | 850.0 | 723.4 | |
| 0.00 | 1.29 | 0.00 | 0.70 | 22.86 | 56.69 | -15.91 | 36.99 | 0.4216 | -815.0 | -641.8 | |
| 0.00 | 2.15 | 0.00 | 1.15 | 19.49 | 56.73 | -15.87 | 42.70 | 0.3818 | 914.0 | 733.5 | |
| 0.00 | 2.24 | 0.00 | 1.21 | 20.20 | 56.36 | -16.24 | 42.02 | 0.3938 | 662.0 | 653.3 | |
| 0.00 | 0.95 | 0.00 | 0.51 | 18.80 | 56.24 | -16.36 | 44.85 | 0.3796 | 859.0 | 712.6 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 17.94 | 56.07 | -16.53 | 46.89 | 0.3725 | 727.0 | 515.6 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 22.02 | 55.22 | -17.38 | 40.71 | 0.4264 | 827.0 | 659.1 | |
| 0.00 | 1.55 | 0.00 | 0.85 | 22.34 | 54.13 | -18.47 | 41.82 | 0.4414 | 654.0 | 490.8 | |
| 0.69 | 1.46 | 0.38 | 0.81 | 21.65 | 53.82 | -18.78 | 43.42 | 0.4372 | 1022.9 | 890.1 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 22.34 | 53.72 | -18.88 | 42.41 | 0.4456 | 768.0 | 597.4 | |
| 0.00 | 4.30 | 0.00 | 2.36 | 21.33 | 53.79 | -18.81 | 44.00 | 0.4341 | 944.0 | 607.7 | |
| 0.00 | 1.12 | 0.00 | 0.63 | 23.88 | 51.67 | -20.93 | 42.75 | 0.4834 | -651.0 | -541.0 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 21.07 | 51.43 | -21.17 | 47.64 | 0.4581 | 606.0 | 440.1 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 20.21 | 47.77 | -24.83 | 53.23 | 0.4940 | 786.0 | 636.2 | |
| 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. | |