SDO HMI 2011-11-29 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 |
| 77.91 | 213.35 | 41.33 | 113.38 | 18.90 | 170.65 | -11.50 | 31.26 | 0.3621 | -54.9 | 146.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.81 | 78.86 | 3.04 | 41.40 | 18.34 | 173.89 | -8.26 | 24.72 | 0.3278 | -1086.0 | -428.2 | |
| 5.04 | -1.00 | 2.64 | -1.00 | 18.06 | 173.77 | -8.38 | 25.39 | 0.3244 | -1205.0 | 999999 | |
| 28.37 | -1.00 | 14.89 | -1.00 | 18.46 | 173.38 | -8.77 | 25.86 | 0.3332 | -1085.2 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 19.39 | 173.29 | -8.86 | 24.82 | 0.3474 | 528.0 | 365.2 | |
| 0.00 | 1.62 | 0.00 | 0.85 | 17.90 | 172.74 | -9.41 | 28.27 | 0.3298 | -1010.0 | -902.5 | |
| 0.00 | 2.99 | 0.00 | 1.57 | 18.15 | 172.70 | -9.45 | 28.01 | 0.3337 | -636.0 | -624.3 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.64 | 172.64 | -9.51 | 27.43 | 0.3413 | -635.0 | -453.3 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 17.53 | 172.54 | -9.61 | 29.35 | 0.3261 | -702.0 | -463.3 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 18.55 | 172.46 | -9.69 | 28.02 | 0.3414 | -673.0 | -560.0 | |
| 0.68 | 5.81 | 0.36 | 3.05 | 17.84 | 172.46 | -9.69 | 29.07 | 0.3312 | -891.8 | -755.5 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 18.02 | 172.08 | -10.07 | 29.73 | 0.3369 | -796.0 | -566.9 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 18.95 | 171.45 | -10.70 | 29.80 | 0.3550 | -850.0 | -694.0 | |
| 1.28 | 3.25 | 0.68 | 1.71 | 18.17 | 171.18 | -10.97 | 31.60 | 0.3465 | 794.2 | 796.4 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 18.89 | 171.04 | -11.11 | 30.81 | 0.3575 | -562.0 | -469.7 | |
| 1.97 | 2.48 | 1.04 | 1.31 | 18.20 | 170.83 | -11.32 | 32.35 | 0.3500 | -839.5 | -716.5 | |
| 0.00 | 2.05 | 0.00 | 1.09 | 18.61 | 170.68 | -11.47 | 32.06 | 0.3568 | -667.0 | -490.4 | |
| 2.56 | 3.76 | 1.37 | 2.01 | 19.79 | 169.76 | -12.39 | 32.20 | 0.3806 | -829.6 | -745.1 | |
| 0.00 | 3.25 | 0.00 | 1.73 | 18.73 | 169.68 | -12.47 | 34.01 | 0.3673 | 1107.0 | 857.2 | |
| 1.11 | 3.93 | 0.59 | 2.10 | 18.97 | 169.50 | -12.65 | 33.98 | 0.3722 | 826.5 | 654.6 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 19.32 | 169.28 | -12.87 | 33.89 | 0.3786 | 832.0 | 563.4 | |
| 0.00 | 2.05 | 0.00 | 1.10 | 19.04 | 169.14 | -13.01 | 34.61 | 0.3762 | 1089.0 | 867.0 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 18.63 | 169.05 | -13.10 | 35.47 | 0.3719 | 843.0 | 719.4 | |
| 0.00 | 5.38 | 0.00 | 2.88 | 19.31 | 168.99 | -13.16 | 34.47 | 0.3813 | 1058.0 | 764.6 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 20.59 | 168.72 | -13.43 | 33.06 | 0.4004 | 671.0 | 621.0 | |
| 2.90 | 63.39 | 1.56 | 34.04 | 19.16 | 168.71 | -13.44 | 35.27 | 0.3818 | 1165.0 | 581.8 | |
| 2.65 | 3.33 | 1.42 | 1.78 | 18.75 | 168.55 | -13.60 | 36.24 | 0.3782 | 1008.6 | 787.5 | |
| 9.14 | -25.00 | 4.90 | -25.00 | 19.22 | 168.39 | -13.76 | 35.81 | 0.3857 | 1125.2 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 20.06 | 168.05 | -14.10 | 35.12 | 0.3995 | 1120.0 | 906.1 | |
| 6.75 | -25.00 | 3.63 | -25.00 | 19.37 | 168.05 | -14.10 | 36.20 | 0.3908 | 833.9 | 999999 | |
| 3.93 | 11.45 | 2.13 | 6.20 | 20.34 | 167.86 | -14.29 | 35.04 | 0.4048 | 990.0 | 689.9 | |
| 5.72 | -25.00 | 3.08 | -25.00 | 19.15 | 167.78 | -14.37 | 37.07 | 0.3907 | 884.8 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 20.37 | 167.60 | -14.55 | 35.47 | 0.4076 | 651.0 | 544.6 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 20.21 | 167.45 | -14.70 | 35.98 | 0.4070 | 950.0 | 792.2 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 20.15 | 167.20 | -14.95 | 36.54 | 0.4086 | 773.0 | 593.9 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 19.27 | 166.50 | -15.65 | 39.17 | 0.4048 | 933.0 | 735.9 | |
| 0.00 | 1.54 | 0.00 | 0.84 | 19.93 | 166.34 | -15.81 | 38.39 | 0.4142 | 659.0 | 472.5 | |
| 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. | |