SDO HMI 2011-05-28 18:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.11 | 397.87 | 52.64 | 235.90 | 20.77 | 131.71 | 25.53 | 312.78 | 0.5499 | -69.3 | -157.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.53 | 246.71 | 0.93 | 148.71 | 21.34 | 133.97 | 27.79 | 311.19 | 0.5792 | -770.2 | -411.1 | |
| 1.98 | -1.00 | 1.20 | -1.00 | 20.98 | 133.71 | 27.53 | 310.92 | 0.5733 | -723.6 | 999999 | |
| 8.93 | -1.00 | 5.42 | -1.00 | 21.64 | 133.77 | 27.59 | 311.78 | 0.5796 | -906.4 | 999999 | |
| 4.60 | -1.00 | 2.77 | -1.00 | 20.72 | 133.51 | 27.33 | 310.74 | 0.5689 | -1105.5 | 999999 | |
| 0.99 | 2.71 | 0.59 | 1.61 | 19.80 | 133.19 | 27.01 | 309.72 | 0.5577 | -818.4 | -874.6 | |
| 22.01 | -1.00 | 13.25 | -1.00 | 21.04 | 133.36 | 27.18 | 311.35 | 0.5700 | -1069.7 | 999999 | |
| 2.35 | -1.00 | 1.40 | -1.00 | 20.65 | 133.06 | 26.88 | 311.08 | 0.5634 | -1251.6 | 999999 | |
| 1.62 | -1.00 | 0.97 | -1.00 | 20.97 | 132.39 | 26.21 | 312.21 | 0.5590 | -831.5 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 21.36 | 132.11 | 25.93 | 313.06 | 0.5594 | -848.0 | -709.0 | |
| 0.00 | 0.72 | 0.00 | 0.43 | 21.26 | 131.76 | 25.58 | 313.27 | 0.5548 | -738.0 | -565.4 | |
| 3.25 | 7.22 | 1.92 | 4.27 | 21.09 | 131.55 | 25.37 | 313.26 | 0.5510 | -893.3 | -790.5 | |
| 1.80 | 6.40 | 1.05 | 3.74 | 19.10 | 131.20 | 25.02 | 310.70 | 0.5293 | 693.2 | 430.5 | |
| 0.45 | -11.00 | 0.27 | -11.00 | 20.93 | 131.41 | 25.23 | 313.18 | 0.5481 | -931.6 | 999999 | |
| 1.98 | 26.52 | 1.15 | 15.46 | 19.16 | 130.86 | 24.68 | 311.17 | 0.5260 | 798.7 | 578.7 | |
| 15.88 | -14.00 | 9.26 | -14.00 | 19.65 | 130.80 | 24.62 | 311.97 | 0.5297 | 843.8 | 999999 | |
| 0.00 | 1.53 | 0.00 | 0.90 | 20.17 | 130.85 | 24.67 | 312.69 | 0.5350 | -308.0 | -231.2 | |
| 0.00 | 1.26 | 0.00 | 0.74 | 20.56 | 130.84 | 24.66 | 313.26 | 0.5386 | -633.0 | -506.8 | |
| 0.00 | 5.41 | 0.00 | 3.13 | 19.45 | 129.99 | 23.81 | 312.57 | 0.5189 | 672.0 | 654.1 | |
| 0.00 | 1.71 | 0.00 | 1.00 | 20.88 | 130.01 | 23.83 | 314.66 | 0.5327 | 654.0 | 357.8 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 13.26 | 128.92 | 22.74 | 303.25 | 0.4518 | -644.0 | -576.3 | |
| 0.00 | 1.98 | 0.00 | 1.14 | 19.25 | 129.39 | 23.21 | 312.96 | 0.5105 | 1062.0 | 798.2 | |
| 0.00 | 0.72 | 0.00 | 0.41 | 19.21 | 129.21 | 23.03 | 313.12 | 0.5081 | 829.0 | 606.6 | |
| 0.00 | 1.26 | 0.00 | 0.72 | 18.76 | 128.97 | 22.79 | 312.70 | 0.5011 | 846.0 | 718.1 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 20.48 | 129.02 | 22.84 | 315.23 | 0.5184 | -109.0 | -114.5 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 16.95 | 128.14 | 21.96 | 310.80 | 0.4745 | -633.0 | -466.1 | |
| 5.23 | 8.57 | 3.02 | 4.94 | 20.74 | 128.46 | 22.28 | 316.28 | 0.5152 | 769.7 | 639.7 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 19.69 | 128.10 | 21.92 | 315.20 | 0.5007 | 696.0 | 609.2 | |
| 1.98 | 2.89 | 1.14 | 1.66 | 20.57 | 128.05 | 21.87 | 316.55 | 0.5092 | 741.6 | 706.6 | |
| 0.00 | 2.89 | 0.00 | 1.65 | 19.79 | 127.90 | 21.72 | 315.59 | 0.4996 | 731.0 | 629.8 | |
| 0.00 | 1.35 | 0.00 | 0.77 | 20.11 | 127.88 | 21.70 | 316.10 | 0.5027 | 728.0 | 572.6 | |
| 0.00 | 2.71 | 0.00 | 1.55 | 20.31 | 127.77 | 21.59 | 316.53 | 0.5035 | 935.0 | 786.7 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 17.30 | 127.36 | 21.18 | 312.36 | 0.4688 | -696.0 | -556.2 | |
| 2.62 | 68.47 | 1.50 | 39.15 | 20.43 | 127.40 | 21.22 | 317.18 | 0.5011 | 932.4 | 431.3 | |
| 11.91 | -33.00 | 6.80 | -33.00 | 20.63 | 127.01 | 20.83 | 317.97 | 0.4991 | 1097.5 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 20.04 | 126.69 | 20.51 | 317.54 | 0.4895 | 676.0 | 551.4 | |
| 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. | |