SDO HMI 2011-10-13 01:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.72 | 201.89 | 46.30 | 133.54 | 9.96 | 49.59 | -41.59 | 81.79 | 0.6621 | -59.5 | -82.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.17 | 82.59 | 4.52 | 52.54 | 9.91 | 52.86 | -38.32 | 81.65 | 0.6197 | -993.6 | -430.0 | |
| 4.20 | -1.00 | 2.66 | -1.00 | 10.03 | 52.41 | -38.77 | 81.49 | 0.6258 | -871.3 | 999999 | |
| 5.51 | -1.00 | 3.50 | -1.00 | 9.78 | 52.29 | -38.89 | 81.90 | 0.6272 | -862.7 | 999999 | |
| 15.14 | -1.00 | 9.64 | -1.00 | 9.55 | 52.01 | -39.17 | 82.28 | 0.6309 | -978.5 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.73 | 9.07 | 51.60 | -39.58 | 83.06 | 0.6361 | -486.0 | -451.5 | |
| 0.00 | 1.75 | 0.00 | 1.12 | 9.31 | 51.45 | -39.73 | 82.70 | 0.6382 | -632.0 | -563.8 | |
| 0.00 | 3.59 | 0.00 | 2.31 | 9.60 | 51.30 | -39.89 | 82.26 | 0.6404 | 119.0 | 48.3 | |
| 0.96 | 4.81 | 0.62 | 3.10 | 9.10 | 51.13 | -40.06 | 83.03 | 0.6425 | -447.3 | -526.2 | |
| 1.49 | 19.77 | 0.97 | 12.97 | 10.43 | 50.21 | -40.97 | 81.04 | 0.6552 | -610.1 | -186.6 | |
| 2.10 | -9.00 | 1.38 | -9.00 | 10.11 | 49.98 | -41.21 | 81.54 | 0.6580 | 510.4 | 999999 | |
| 2.45 | 11.90 | 1.61 | 7.84 | 9.61 | 49.77 | -41.42 | 82.31 | 0.6605 | 757.2 | 122.5 | |
| 0.00 | 2.27 | 0.00 | 1.49 | 8.81 | 49.88 | -41.30 | 83.53 | 0.6587 | -758.0 | -557.8 | |
| 2.54 | 4.37 | 1.68 | 2.90 | 10.66 | 49.27 | -41.91 | 80.75 | 0.6674 | -613.9 | -507.4 | |
| 0.00 | 0.96 | 0.00 | 0.64 | 10.40 | 49.32 | -41.86 | 81.15 | 0.6666 | -705.0 | -563.2 | |
| 0.00 | 1.92 | 0.00 | 1.28 | 10.25 | 49.01 | -42.17 | 81.38 | 0.6705 | -513.0 | -442.7 | |
| 0.00 | 1.05 | 0.00 | 0.70 | 8.73 | 49.20 | -41.98 | 83.66 | 0.6675 | -482.0 | -427.8 | |
| 0.00 | 0.61 | 0.00 | 0.41 | 9.74 | 48.97 | -42.21 | 82.16 | 0.6708 | -544.0 | -467.1 | |
| 0.00 | 1.22 | 0.00 | 0.82 | 8.79 | 48.83 | -42.36 | 83.57 | 0.6724 | -439.0 | -322.9 | |
| 2.10 | 5.69 | 1.41 | 3.83 | 9.18 | 48.27 | -42.91 | 83.01 | 0.6795 | 693.4 | 440.5 | |
| 0.00 | 0.96 | 0.00 | 0.65 | 10.51 | 47.89 | -43.29 | 81.08 | 0.6848 | -336.0 | -322.3 | |
| 0.00 | 1.92 | 0.00 | 1.32 | 11.45 | 47.17 | -44.02 | 79.75 | 0.6944 | 930.0 | 752.0 | |
| 2.19 | 4.55 | 1.51 | 3.14 | 10.95 | 46.88 | -44.31 | 80.50 | 0.6976 | 757.0 | 659.0 | |
| 1.22 | 7.17 | 0.84 | 4.94 | 9.70 | 46.80 | -44.38 | 82.29 | 0.6981 | 869.4 | 563.8 | |
| 2.62 | 18.29 | 1.83 | 12.79 | 9.82 | 46.27 | -44.91 | 82.15 | 0.7046 | 725.9 | 659.9 | |
| 0.00 | 1.14 | 0.00 | 0.79 | 10.71 | 46.11 | -45.08 | 80.88 | 0.7070 | 803.0 | 568.2 | |
| 2.71 | -24.00 | 1.89 | -24.00 | 10.02 | 46.15 | -45.04 | 81.86 | 0.7062 | 963.0 | 999999 | |
| 0.00 | 1.31 | 0.00 | 0.92 | 10.68 | 45.76 | -45.42 | 80.94 | 0.7111 | 705.0 | 632.9 | |
| 7.00 | -24.00 | 4.91 | -24.00 | 10.14 | 45.82 | -45.36 | 81.70 | 0.7102 | 861.9 | 999999 | |
| 0.00 | 1.84 | 0.00 | 1.29 | 11.07 | 45.64 | -45.54 | 80.40 | 0.7127 | 622.0 | 508.3 | |
| 0.00 | 0.26 | 0.00 | 0.18 | 10.76 | 45.57 | -45.61 | 80.84 | 0.7134 | 232.0 | 329.0 | |
| 1.22 | 2.10 | 0.86 | 1.48 | 10.58 | 45.57 | -45.62 | 81.10 | 0.7134 | 839.5 | 749.6 | |
| 0.00 | 1.05 | 0.00 | 0.74 | 10.53 | 45.36 | -45.83 | 81.17 | 0.7160 | 743.0 | 677.5 | |
| 0.00 | 1.57 | 0.00 | 1.11 | 10.17 | 45.38 | -45.80 | 81.67 | 0.7155 | 475.0 | 339.2 | |
| 3.59 | 13.82 | 2.55 | 9.83 | 10.91 | 45.11 | -46.08 | 80.66 | 0.7191 | 583.1 | 479.1 | |
| 5.51 | -34.00 | 3.92 | -34.00 | 10.60 | 44.99 | -46.19 | 81.10 | 0.7203 | 635.0 | 999999 | |
| 0.00 | 1.40 | 0.00 | 1.01 | 10.59 | 44.46 | -46.72 | 81.13 | 0.7266 | 274.0 | 263.8 | |
| 0.00 | 0.87 | 0.00 | 0.67 | 12.15 | 41.20 | -49.99 | 79.19 | 0.7646 | 415.0 | 331.0 | |
| 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. | |