SDO HMI 2011-09-01 21:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 103.84 | 432.18 | 59.40 | 247.97 | 24.55 | 300.16 | 25.59 | 308.60 | 0.5041 | -1.2 | -49.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.04 | 199.72 | 14.67 | 116.93 | 23.46 | 303.56 | 28.99 | 303.51 | 0.5353 | -1058.2 | -358.7 | |
| 7.60 | -1.00 | 4.44 | -1.00 | 23.09 | 303.40 | 28.82 | 303.01 | 0.5309 | -1345.0 | 999999 | |
| 3.04 | -1.00 | 1.78 | -1.00 | 23.71 | 303.20 | 28.63 | 304.19 | 0.5325 | -1118.7 | 999999 | |
| 3.94 | 5.28 | 2.31 | 3.10 | 24.68 | 303.41 | 28.83 | 305.66 | 0.5414 | -685.8 | -518.7 | |
| 0.00 | 2.15 | 0.00 | 1.27 | 25.82 | 303.70 | 29.13 | 307.27 | 0.5528 | 533.0 | 551.8 | |
| 0.00 | 1.52 | 0.00 | 0.87 | 20.57 | 302.44 | 27.87 | 299.22 | 0.5034 | -848.0 | -696.6 | |
| 8.32 | -1.00 | 4.85 | -1.00 | 23.69 | 302.94 | 28.36 | 304.37 | 0.5291 | -1096.9 | 999999 | |
| 0.00 | 1.34 | 0.00 | 0.79 | 24.45 | 302.93 | 28.36 | 305.66 | 0.5342 | -490.0 | -416.8 | |
| 0.00 | 6.80 | 0.00 | 3.96 | 24.28 | 302.66 | 28.09 | 305.58 | 0.5298 | -748.0 | -604.5 | |
| 0.00 | 1.34 | 0.00 | 0.77 | 23.40 | 301.93 | 27.36 | 304.67 | 0.5149 | -889.0 | -797.2 | |
| 2.24 | 11.63 | 1.29 | 6.71 | 24.34 | 301.52 | 26.94 | 306.64 | 0.5165 | -721.3 | -579.3 | |
| 0.00 | 0.89 | 0.00 | 0.51 | 22.13 | 300.24 | 25.66 | 303.84 | 0.4850 | -671.0 | -562.7 | |
| 0.00 | 0.72 | 0.00 | 0.41 | 23.10 | 300.40 | 25.82 | 305.46 | 0.4939 | 645.0 | 575.4 | |
| 0.00 | 1.07 | 0.00 | 0.62 | 24.55 | 300.49 | 25.91 | 307.92 | 0.5059 | -666.0 | -575.1 | |
| 0.89 | 9.39 | 0.51 | 5.33 | 23.41 | 299.88 | 25.30 | 306.49 | 0.4898 | 713.4 | 502.6 | |
| 3.22 | 12.88 | 1.84 | 7.37 | 24.94 | 299.91 | 25.33 | 309.12 | 0.5021 | -846.4 | -471.8 | |
| 1.34 | 8.85 | 0.77 | 5.08 | 25.52 | 299.81 | 25.24 | 310.18 | 0.5057 | -666.0 | -680.0 | |
| 0.00 | 2.06 | 0.00 | 1.17 | 23.85 | 299.35 | 24.77 | 307.77 | 0.4868 | 833.0 | 814.0 | |
| 0.00 | 1.07 | 0.00 | 0.61 | 24.06 | 299.02 | 24.45 | 308.46 | 0.4846 | 744.0 | 593.2 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 25.22 | 298.79 | 24.22 | 310.70 | 0.4914 | -535.0 | -437.0 | |
| 0.00 | 1.97 | 0.00 | 1.11 | 24.58 | 298.07 | 23.50 | 310.35 | 0.4778 | 834.0 | 598.0 | |
| 3.58 | 5.28 | 2.01 | 2.96 | 24.97 | 297.21 | 22.64 | 311.98 | 0.4712 | 818.0 | 590.4 | |
| 4.56 | 6.53 | 2.55 | 3.66 | 25.11 | 296.84 | 22.27 | 312.65 | 0.4683 | 943.4 | 578.4 | |
| 0.00 | 1.61 | 0.00 | 0.91 | 27.04 | 296.90 | 22.33 | 315.78 | 0.4871 | -39.0 | -34.1 | |
| 2.95 | 40.52 | 1.67 | 22.86 | 26.83 | 296.60 | 22.02 | 315.79 | 0.4818 | 812.0 | 366.9 | |
| 8.05 | -25.00 | 4.53 | -25.00 | 26.64 | 296.38 | 21.80 | 315.75 | 0.4777 | 992.3 | 999999 | |
| 0.00 | 4.11 | 0.00 | 2.33 | 27.16 | 296.45 | 21.87 | 316.50 | 0.4835 | -51.0 | 10.6 | |
| 0.00 | 1.25 | 0.00 | 0.70 | 26.20 | 296.22 | 21.64 | 315.21 | 0.4717 | 701.0 | 510.9 | |
| 0.00 | 3.94 | 0.00 | 2.20 | 25.79 | 295.96 | 21.38 | 314.85 | 0.4649 | 774.0 | 626.6 | |
| 0.00 | 2.06 | 0.00 | 1.15 | 26.02 | 295.89 | 21.32 | 315.31 | 0.4664 | 679.0 | 558.9 | |
| 2.86 | -25.00 | 1.61 | -25.00 | 26.82 | 295.98 | 21.40 | 316.52 | 0.4752 | 718.5 | 999999 | |
| 0.00 | 5.10 | 0.00 | 2.86 | 26.61 | 295.64 | 21.07 | 316.59 | 0.4696 | 1027.0 | 703.0 | |
| 26.21 | 85.32 | 14.57 | 47.39 | 25.70 | 295.18 | 20.61 | 315.64 | 0.4556 | 1156.5 | 565.3 | |
| 0.00 | 3.94 | 0.00 | 2.20 | 26.60 | 295.10 | 20.53 | 317.25 | 0.4638 | 770.0 | 608.4 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 25.45 | 294.14 | 19.57 | 316.59 | 0.4419 | 932.0 | 747.5 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 25.49 | 293.93 | 19.36 | 316.94 | 0.4401 | 757.0 | 569.5 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 26.49 | 293.96 | 19.39 | 318.56 | 0.4508 | 731.0 | 561.2 | |
| 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. | |