SDO HMI 2011-12-05 09:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.61 | 187.98 | 15.52 | 98.66 | 18.97 | 103.48 | -4.55 | 13.09 | 0.3301 | -440.5 | -302.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.75 | 17.59 | 108.29 | 0.27 | 359.15 | 0.2975 | -813.0 | -547.7 | |
| 29.61 | 169.21 | 15.52 | 88.71 | 18.99 | 103.92 | -4.11 | 11.98 | 0.3279 | -1301.9 | -403.4 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 19.86 | 102.98 | -5.04 | 13.92 | 0.3454 | -725.0 | -531.6 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 15.65 | 101.34 | -6.68 | 23.03 | 0.2878 | 924.0 | 633.2 | |
| 0.00 | 2.30 | 0.00 | 1.19 | 15.10 | 101.30 | -6.73 | 23.97 | 0.2796 | 635.0 | 407.1 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 14.31 | 101.29 | -6.73 | 25.24 | 0.2676 | 918.0 | 803.0 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 16.63 | 101.16 | -6.87 | 22.26 | 0.3041 | 825.0 | 532.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 13.85 | 101.09 | -6.93 | 26.68 | 0.2622 | 822.0 | 671.2 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 18.12 | 100.22 | -7.81 | 22.95 | 0.3326 | 893.0 | 662.1 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 18.21 | 99.15 | -8.88 | 25.57 | 0.3412 | 846.0 | 657.9 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 21.28 | 98.17 | -9.86 | 24.08 | 0.3927 | 699.0 | 571.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 18.64 | 97.93 | -10.10 | 27.92 | 0.3566 | 909.0 | 685.5 | |
| 0.00 | 3.93 | 0.00 | 2.15 | 22.90 | 95.80 | -12.23 | 26.97 | 0.4320 | 928.0 | 624.7 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 22.29 | 94.38 | -13.65 | 30.30 | 0.4345 | 780.0 | 504.8 | |
| 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. | |