SDO HMI 2011-12-05 14:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.22 | 86.57 | 26.24 | 110.87 | 18.81 | 171.19 | 65.91 | 290.38 | 0.9212 | -107.9 | 83.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.35 | 21.58 | 6.81 | 34.23 | 18.92 | 175.90 | 70.62 | 289.86 | 0.9502 | -382.3 | 89.8 | |
| 0.00 | 3.16 | 0.00 | 4.84 | 19.14 | 175.46 | 70.17 | 290.14 | 0.9480 | -552.0 | -475.1 | |
| 4.61 | 7.93 | 6.51 | 11.20 | 18.99 | 173.62 | 68.34 | 290.19 | 0.9379 | -405.6 | -273.8 | |
| 0.00 | 2.13 | 0.00 | 2.71 | 18.34 | 171.15 | 65.87 | 289.83 | 0.9225 | -537.0 | -365.6 | |
| 1.36 | 2.30 | 1.66 | 2.80 | 17.51 | 170.11 | 64.82 | 289.07 | 0.9149 | -461.9 | -484.5 | |
| 3.33 | 5.37 | 4.08 | 6.59 | 17.94 | 170.26 | 64.97 | 289.52 | 0.9163 | -466.5 | -415.3 | |
| 0.00 | 0.51 | 0.00 | 0.64 | 18.53 | 170.53 | 65.25 | 290.12 | 0.9187 | -356.0 | -348.3 | |
| 0.00 | 1.71 | 0.00 | 2.08 | 20.48 | 169.71 | 64.42 | 292.35 | 0.9154 | 359.0 | 224.4 | |
| 0.00 | 1.11 | 0.00 | 1.26 | 18.67 | 168.04 | 62.75 | 290.65 | 0.9019 | 317.0 | 181.8 | |
| 0.00 | 4.61 | 0.00 | 5.14 | 18.17 | 167.58 | 62.30 | 290.18 | 0.8981 | 445.0 | 242.2 | |
| 2.73 | 33.69 | 3.00 | 36.70 | 18.70 | 166.98 | 61.70 | 290.87 | 0.8944 | 483.1 | 262.4 | |
| 3.84 | -11.00 | 4.18 | -11.00 | 18.96 | 166.68 | 61.39 | 291.20 | 0.8925 | 636.6 | 999999 | |
| 0.00 | 2.47 | 0.00 | 2.68 | 19.40 | 166.50 | 61.22 | 291.72 | 0.8918 | 541.0 | 476.0 | |
| 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. | |