SDO HMI 2011-12-09 10:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.18 | 520.88 | 65.09 | 462.16 | -22.76 | 107.82 | 53.05 | 242.38 | 0.8337 | 541.5 | 289.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.70 | 7.50 | 1.62 | 7.08 | -17.71 | 111.53 | 56.76 | 249.19 | 0.8544 | 485.4 | 566.3 | |
| 0.00 | 0.51 | 0.00 | 0.48 | -17.46 | 111.41 | 56.64 | 249.45 | 0.8530 | 613.0 | 562.8 | |
| 1.36 | -1.00 | 1.28 | -1.00 | -17.61 | 111.26 | 56.49 | 249.24 | 0.8520 | 743.6 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.81 | -20.49 | 107.25 | 52.48 | 244.86 | 0.8228 | -236.0 | -228.3 | |
| 2.22 | 457.66 | 2.01 | 408.89 | -23.23 | 108.56 | 53.79 | 242.07 | 0.8413 | 420.5 | 339.2 | |
| 64.26 | -5.00 | 57.85 | -5.00 | -22.94 | 108.12 | 53.35 | 242.27 | 0.8369 | 944.3 | 999999 | |
| 0.00 | 6.05 | 0.00 | 5.22 | -21.19 | 106.81 | 52.04 | 243.91 | 0.8208 | 256.0 | 244.4 | |
| 1.62 | -5.00 | 1.45 | -5.00 | -23.49 | 107.85 | 53.07 | 241.55 | 0.8360 | 574.6 | 999999 | |
| 0.00 | 1.19 | 0.00 | 1.02 | -21.48 | 106.39 | 51.62 | 243.44 | 0.8177 | 248.0 | 318.3 | |
| 0.00 | 1.11 | 0.00 | 0.94 | -21.60 | 106.20 | 51.42 | 243.23 | 0.8164 | 534.0 | 429.8 | |
| 0.00 | 2.05 | 0.00 | 1.70 | -20.06 | 105.36 | 50.59 | 244.81 | 0.8043 | -567.0 | -451.5 | |
| 0.00 | 1.02 | 0.00 | 0.84 | -19.74 | 105.03 | 50.25 | 245.08 | 0.8002 | -604.0 | -505.7 | |
| 1.02 | -5.00 | 0.88 | -5.00 | -22.88 | 106.45 | 51.67 | 241.81 | 0.8222 | 680.1 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.20 | -20.78 | 105.09 | 50.32 | 243.85 | 0.8039 | -494.0 | -429.0 | |
| 0.00 | 1.79 | 0.00 | 1.47 | -20.40 | 104.63 | 49.85 | 244.15 | 0.7984 | -577.0 | -527.0 | |
| 0.00 | 2.73 | 0.00 | 2.39 | -24.72 | 106.38 | 51.61 | 239.66 | 0.8272 | 583.0 | 436.3 | |
| 0.00 | 1.87 | 0.00 | 1.59 | -23.11 | 105.33 | 50.56 | 241.17 | 0.8130 | 206.0 | 205.4 | |
| 0.00 | 10.40 | 0.00 | 8.62 | -22.15 | 104.65 | 49.87 | 242.07 | 0.8038 | -83.0 | 6.9 | |
| 0.00 | 1.45 | 0.00 | 1.19 | -21.83 | 104.44 | 49.67 | 242.38 | 0.8010 | -432.0 | -400.1 | |
| 0.00 | 5.03 | 0.00 | 4.26 | -23.56 | 105.26 | 50.49 | 240.62 | 0.8139 | -182.0 | 13.7 | |
| 0.00 | 1.28 | 0.00 | 1.08 | -23.33 | 105.15 | 50.37 | 240.84 | 0.8121 | -305.0 | -164.4 | |
| 0.00 | 0.85 | 0.00 | 0.71 | -23.01 | 104.83 | 50.06 | 241.11 | 0.8082 | -268.0 | -180.3 | |
| 0.00 | 1.70 | 0.00 | 1.40 | -21.86 | 104.21 | 49.44 | 242.26 | 0.7989 | -477.0 | -380.6 | |
| 0.00 | 2.64 | 0.00 | 2.18 | -22.43 | 104.34 | 49.57 | 241.62 | 0.8019 | -174.0 | -194.8 | |
| 0.00 | 1.02 | 0.00 | 0.81 | -19.55 | 103.06 | 48.29 | 244.66 | 0.7807 | -470.0 | -394.2 | |
| 0.00 | 0.34 | 0.00 | 0.28 | -21.10 | 103.72 | 48.94 | 243.01 | 0.7918 | -461.0 | -532.8 | |
| 0.00 | 1.11 | 0.00 | 0.87 | -19.93 | 102.84 | 48.07 | 244.12 | 0.7796 | -566.0 | -457.5 | |
| 0.00 | 1.19 | 0.00 | 0.94 | -20.62 | 102.84 | 48.07 | 243.27 | 0.7819 | -633.0 | -601.1 | |
| 0.00 | 0.85 | 0.00 | 0.66 | -19.46 | 102.37 | 47.60 | 244.54 | 0.7734 | -501.0 | -518.0 | |
| 0.00 | 0.85 | 0.00 | 0.66 | -19.46 | 102.04 | 47.27 | 244.42 | 0.7702 | -564.0 | -505.6 | |
| 0.00 | 1.45 | 0.00 | 1.12 | -20.06 | 101.72 | 46.95 | 243.56 | 0.7689 | -617.0 | -496.2 | |
| 0.00 | 1.36 | 0.00 | 1.08 | -22.53 | 102.44 | 47.67 | 240.80 | 0.7845 | -547.0 | -471.9 | |
| 0.00 | 1.02 | 0.00 | 0.82 | -23.14 | 102.58 | 47.81 | 240.12 | 0.7880 | -301.0 | -328.8 | |
| 0.00 | 1.53 | 0.00 | 1.15 | -20.28 | 99.94 | 45.17 | 242.59 | 0.7516 | -594.0 | -537.4 | |
| 0.00 | 0.94 | 0.00 | 0.70 | -20.53 | 99.99 | 45.22 | 242.30 | 0.7531 | -485.0 | -382.4 | |
| 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. | |