SDO HMI 2011-01-05 22:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.29 | 106.89 | 13.02 | 56.80 | -14.51 | 208.11 | 18.06 | 236.74 | 0.3587 | -43.1 | -276.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.97 | 0.00 | 1.63 | -16.39 | 212.27 | 22.21 | 237.99 | 0.4296 | 718.0 | 623.6 | |
| 3.74 | 21.15 | 2.03 | 11.50 | -15.25 | 211.90 | 21.85 | 240.02 | 0.4164 | 841.8 | 584.9 | |
| 2.97 | -2.00 | 1.61 | -2.00 | -14.86 | 211.76 | 21.71 | 240.72 | 0.4117 | 905.1 | 999999 | |
| 11.80 | 17.15 | 6.38 | 9.27 | -14.57 | 211.18 | 21.12 | 240.75 | 0.4015 | 979.9 | 481.3 | |
| 0.00 | 1.44 | 0.00 | 0.78 | -15.69 | 211.07 | 21.01 | 238.16 | 0.4081 | 826.0 | 680.8 | |
| 0.00 | 0.76 | 0.00 | 0.41 | -14.28 | 210.60 | 20.54 | 240.78 | 0.3913 | 840.0 | 689.1 | |
| 0.00 | 2.38 | 0.00 | 1.27 | -13.81 | 210.07 | 20.01 | 241.30 | 0.3805 | 1084.0 | 829.8 | |
| 0.00 | 0.76 | 0.00 | 0.41 | -13.85 | 209.81 | 19.76 | 240.93 | 0.3772 | 767.0 | 597.6 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -16.50 | 209.68 | 19.63 | 234.74 | 0.3961 | 791.0 | 531.4 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -13.44 | 207.60 | 17.55 | 239.21 | 0.3429 | -777.0 | -571.5 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -13.65 | 207.58 | 17.53 | 238.65 | 0.3443 | -554.0 | -487.6 | |
| 0.00 | 4.08 | 0.00 | 2.15 | -15.35 | 206.64 | 16.58 | 233.04 | 0.3460 | -749.0 | -560.6 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -14.54 | 206.41 | 16.36 | 234.67 | 0.3357 | -720.0 | -528.7 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -15.21 | 206.31 | 16.25 | 232.86 | 0.3403 | -759.0 | -613.6 | |
| 0.00 | 1.70 | 0.00 | 0.89 | -15.12 | 206.11 | 16.06 | 232.75 | 0.3369 | -762.0 | -632.8 | |
| 0.00 | 7.47 | 0.00 | 3.91 | -13.65 | 205.84 | 15.79 | 236.08 | 0.3201 | -503.0 | -648.2 | |
| 0.00 | 8.15 | 0.00 | 4.27 | -14.40 | 205.71 | 15.65 | 233.89 | 0.3249 | -672.0 | -776.5 | |
| 0.00 | 0.93 | 0.00 | 0.49 | -13.99 | 205.65 | 15.59 | 234.88 | 0.3203 | -870.0 | -660.0 | |
| 0.00 | 1.10 | 0.00 | 0.58 | -14.50 | 205.46 | 15.41 | 233.23 | 0.3225 | -859.0 | -696.8 | |
| 0.00 | 14.61 | 0.00 | 7.62 | -13.93 | 205.20 | 15.15 | 234.27 | 0.3138 | -917.0 | -927.2 | |
| 2.38 | 3.31 | 1.24 | 1.73 | -14.48 | 204.92 | 14.87 | 232.35 | 0.3152 | -943.5 | -797.5 | |
| 0.00 | 1.70 | 0.00 | 0.88 | -14.18 | 204.87 | 14.82 | 233.05 | 0.3117 | -963.0 | -787.8 | |
| 0.00 | 3.65 | 0.00 | 1.90 | -14.12 | 204.52 | 14.47 | 232.56 | 0.3065 | -1181.0 | -940.8 | |
| 3.40 | 3.48 | 1.76 | 1.81 | -13.53 | 204.39 | 14.34 | 233.95 | 0.2991 | -973.0 | -1031.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | -13.86 | 204.29 | 14.23 | 232.85 | 0.3009 | -866.0 | -705.5 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -14.13 | 204.15 | 14.09 | 231.85 | 0.3016 | -915.0 | -730.4 | |
| 0.00 | 1.87 | 0.00 | 0.96 | -14.31 | 201.45 | 11.39 | 225.50 | 0.2696 | -1003.0 | -797.4 | |
| 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. | |