SDO HMI 2011-10-04 23:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.81 | 364.17 | 39.48 | 248.62 | 23.20 | 156.09 | -41.74 | 62.90 | 0.6895 | -866.2 | -325.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.81 | 23.58 | 159.13 | -38.70 | 61.15 | 0.6566 | -636.0 | -524.7 | |
| 0.00 | 1.14 | 0.00 | 0.79 | 26.51 | 156.59 | -41.24 | 58.14 | 0.6969 | -777.0 | -726.4 | |
| 0.00 | 1.14 | 0.00 | 0.79 | 26.49 | 156.28 | -41.55 | 58.30 | 0.7000 | -655.0 | -485.9 | |
| 13.27 | 287.37 | 8.95 | 194.64 | 22.65 | 156.73 | -41.10 | 63.44 | 0.6805 | -1162.8 | -372.4 | |
| 27.24 | -4.00 | 18.50 | -4.00 | 23.13 | 156.38 | -41.45 | 62.89 | 0.6862 | -1097.6 | 999999 | |
| 2.28 | -4.00 | 1.54 | -4.00 | 22.25 | 156.44 | -41.39 | 64.12 | 0.6825 | -819.4 | 999999 | |
| 10.90 | 66.26 | 7.58 | 46.32 | 24.11 | 155.06 | -42.77 | 62.01 | 0.7042 | -972.2 | -183.6 | |
| 1.49 | -7.00 | 1.04 | -7.00 | 24.02 | 154.69 | -43.14 | 62.26 | 0.7079 | -724.8 | 999999 | |
| 0.53 | -7.00 | 0.37 | -7.00 | 23.73 | 154.59 | -43.24 | 62.70 | 0.7081 | -549.7 | 999999 | |
| 1.05 | 1.58 | 0.71 | 1.07 | 19.87 | 155.58 | -42.25 | 67.79 | 0.6853 | 476.7 | 383.8 | |
| 1.05 | 1.41 | 0.79 | 1.06 | 24.75 | 150.41 | -47.42 | 62.66 | 0.7551 | 673.2 | 609.2 | |
| 0.00 | 0.70 | 0.00 | 0.52 | 22.65 | 150.54 | -47.29 | 65.35 | 0.7484 | 712.0 | 618.6 | |
| 0.00 | 2.20 | 0.00 | 1.72 | 26.19 | 148.69 | -49.14 | 61.31 | 0.7760 | 652.0 | 556.8 | |
| 0.00 | 1.14 | 0.00 | 0.90 | 26.43 | 148.49 | -49.34 | 61.06 | 0.7785 | 424.0 | 302.6 | |
| 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. | |