SDO HMI 2011-12-02 18:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.11 | 189.88 | 17.27 | 126.11 | 19.43 | 104.51 | -38.10 | 60.98 | 0.6680 | -649.7 | -284.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.13 | 0.00 | 1.44 | 23.72 | 105.45 | -37.16 | 54.60 | 0.6808 | -832.0 | -678.7 | |
| 0.00 | 1.79 | 0.00 | 1.21 | 23.62 | 104.96 | -37.66 | 55.03 | 0.6854 | -669.0 | -457.5 | |
| 0.00 | 1.02 | 0.00 | 0.72 | 24.55 | 103.34 | -39.27 | 54.78 | 0.7072 | -674.0 | -508.2 | |
| 0.00 | 1.37 | 0.00 | 0.93 | 22.05 | 104.13 | -38.48 | 57.59 | 0.6856 | 608.0 | 496.6 | |
| 0.00 | 2.30 | 0.00 | 1.66 | 26.53 | 102.33 | -40.28 | 52.87 | 0.7279 | -669.0 | -571.1 | |
| 0.00 | 1.37 | 0.00 | 0.93 | 21.89 | 103.94 | -38.68 | 57.91 | 0.6868 | 627.0 | 489.5 | |
| 0.00 | 1.02 | 0.00 | 0.67 | 18.16 | 104.97 | -37.64 | 62.50 | 0.6566 | -127.0 | -113.4 | |
| 0.00 | 7.51 | 0.00 | 5.15 | 22.68 | 103.59 | -39.02 | 57.05 | 0.6946 | 337.0 | 135.4 | |
| 25.09 | 166.43 | 16.57 | 109.94 | 18.97 | 104.68 | -37.93 | 61.51 | 0.6638 | -1083.0 | -322.6 | |
| 1.02 | 1.45 | 0.70 | 0.99 | 21.98 | 103.54 | -39.08 | 58.01 | 0.6916 | 569.4 | 446.2 | |
| 0.00 | 1.28 | 0.00 | 0.87 | 20.87 | 103.16 | -39.46 | 59.69 | 0.6902 | -691.0 | -623.1 | |
| 0.00 | 1.02 | 0.00 | 0.71 | 18.14 | 101.30 | -41.31 | 64.28 | 0.6987 | 657.0 | 593.1 | |
| 0.00 | 1.19 | 0.00 | 0.89 | 19.26 | 97.33 | -45.29 | 64.40 | 0.7462 | 611.0 | 486.8 | |
| 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. | |