SDO HMI 2012-10-16 00:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 92.03 | 524.41 | 53.72 | 306.85 | 7.30 | 229.15 | -32.26 | 85.47 | 0.5330 | -745.3 | -317.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.71 | 379.47 | 38.57 | 219.48 | 7.41 | 230.21 | -31.20 | 85.24 | 0.5176 | -1498.4 | -396.9 | |
| 0.70 | 1.48 | 0.41 | 0.87 | 5.02 | 228.55 | -32.86 | 89.72 | 0.5426 | 438.1 | 290.7 | |
| 0.00 | 1.66 | 0.00 | 0.98 | 6.10 | 228.16 | -33.25 | 87.70 | 0.5477 | 865.0 | 666.2 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 4.22 | 228.24 | -33.17 | 91.15 | 0.5480 | 728.0 | 447.2 | |
| 0.00 | 0.35 | 0.00 | 0.21 | 6.16 | 228.05 | -33.36 | 87.59 | 0.5493 | 409.0 | 345.8 | |
| 11.61 | 24.80 | 6.89 | 14.71 | 5.07 | 227.87 | -33.54 | 89.56 | 0.5526 | -996.7 | -706.7 | |
| 2.18 | 24.36 | 1.30 | 14.52 | 6.70 | 227.58 | -33.83 | 86.59 | 0.5561 | -917.0 | -755.1 | |
| 0.00 | 1.66 | 0.00 | 0.99 | 7.20 | 227.35 | -34.05 | 85.70 | 0.5593 | -918.0 | -770.9 | |
| 0.00 | 1.57 | 0.00 | 0.94 | 9.76 | 226.99 | -34.42 | 81.16 | 0.5660 | -589.0 | -464.3 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 4.86 | 227.37 | -34.04 | 89.89 | 0.5599 | -552.0 | -415.2 | |
| 0.00 | 1.48 | 0.00 | 0.89 | 5.07 | 227.32 | -34.08 | 89.51 | 0.5604 | -538.0 | -501.0 | |
| 4.02 | -7.00 | 2.40 | -7.00 | 6.89 | 227.16 | -34.25 | 86.26 | 0.5621 | -671.0 | 999999 | |
| 0.00 | 3.14 | 0.00 | 1.88 | 7.30 | 227.05 | -34.36 | 85.52 | 0.5636 | -841.0 | -721.1 | |
| 0.00 | 13.01 | 0.00 | 7.80 | 8.19 | 226.94 | -34.47 | 83.94 | 0.5656 | 394.0 | 181.7 | |
| 0.00 | 1.31 | 0.00 | 0.78 | 4.85 | 227.12 | -34.29 | 89.89 | 0.5635 | -395.0 | -397.1 | |
| 0.00 | 1.83 | 0.00 | 1.10 | 8.69 | 226.77 | -34.63 | 83.06 | 0.5681 | 326.0 | 286.6 | |
| 0.00 | 0.96 | 0.00 | 0.58 | 4.75 | 226.91 | -34.50 | 90.05 | 0.5667 | -420.0 | -317.8 | |
| 0.00 | 6.37 | 0.00 | 3.83 | 7.34 | 226.65 | -34.76 | 85.46 | 0.5695 | -940.0 | -698.6 | |
| 0.00 | 4.37 | 0.00 | 2.63 | 8.62 | 226.49 | -34.92 | 83.21 | 0.5722 | 446.0 | 500.0 | |
| 0.00 | 2.27 | 0.00 | 1.37 | 8.38 | 226.51 | -34.90 | 83.63 | 0.5717 | 808.0 | 669.3 | |
| 0.00 | 1.31 | 0.00 | 0.80 | 9.18 | 225.83 | -35.58 | 82.29 | 0.5818 | 832.0 | 649.9 | |
| 0.00 | 1.40 | 0.00 | 0.85 | 9.42 | 225.77 | -35.64 | 81.88 | 0.5829 | 869.0 | 717.3 | |
| 2.36 | 9.43 | 1.43 | 5.71 | 7.15 | 225.96 | -35.45 | 85.79 | 0.5792 | -792.4 | -716.4 | |
| 0.00 | 0.70 | 0.00 | 0.43 | 8.75 | 225.66 | -35.75 | 83.04 | 0.5840 | 779.0 | 645.1 | |
| 2.27 | 6.20 | 1.38 | 3.77 | 8.39 | 225.66 | -35.75 | 83.66 | 0.5838 | 810.7 | 862.5 | |
| 0.00 | 2.44 | 0.00 | 1.49 | 7.40 | 225.68 | -35.73 | 85.36 | 0.5832 | 122.0 | -127.3 | |
| 0.00 | 8.47 | 0.00 | 5.16 | 7.97 | 225.59 | -35.82 | 84.39 | 0.5846 | 520.0 | 551.3 | |
| 0.00 | 1.14 | 0.00 | 0.69 | 8.92 | 225.49 | -35.92 | 82.76 | 0.5865 | 678.0 | 464.6 | |
| 0.00 | 1.48 | 0.00 | 0.91 | 6.96 | 225.38 | -36.03 | 86.11 | 0.5874 | -713.0 | -558.1 | |
| 2.18 | 9.87 | 1.34 | 6.05 | 7.22 | 225.21 | -36.20 | 85.66 | 0.5898 | -520.1 | 164.4 | |
| 0.00 | 0.96 | 0.00 | 0.59 | 5.96 | 225.13 | -36.28 | 87.81 | 0.5912 | -593.0 | -361.8 | |
| 0.00 | 2.88 | 0.00 | 1.78 | 8.24 | 224.62 | -36.79 | 83.96 | 0.5982 | 653.0 | 536.1 | |
| 0.00 | 0.96 | 0.00 | 0.60 | 8.57 | 223.67 | -37.74 | 83.45 | 0.6114 | 707.0 | 622.0 | |
| 0.00 | 1.31 | 0.00 | 0.82 | 8.20 | 223.52 | -37.89 | 84.06 | 0.6134 | 770.0 | 596.9 | |
| 0.00 | 0.96 | 0.00 | 0.61 | 5.83 | 222.40 | -39.01 | 87.89 | 0.6289 | 663.0 | 595.6 | |
| 0.00 | 1.66 | 0.00 | 1.08 | 6.32 | 220.71 | -40.70 | 87.04 | 0.6513 | 669.0 | 550.2 | |
| 0.00 | 0.96 | 0.00 | 0.65 | 7.06 | 218.36 | -43.05 | 85.84 | 0.6815 | 422.0 | 415.0 | |
| 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. | |