SDO HMI 2011-11-29 15:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.15 | 224.57 | 33.68 | 120.02 | 18.81 | 170.65 | -13.16 | 34.93 | 0.3754 | -43.3 | 68.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.37 | 174.47 | -9.34 | 27.41 | 0.3360 | -721.0 | -576.9 | |
| 1.20 | 86.39 | 0.63 | 45.57 | 18.25 | 173.88 | -9.93 | 29.05 | 0.3388 | -1135.5 | -504.6 | |
| 4.02 | -2.00 | 2.12 | -2.00 | 18.40 | 173.74 | -10.07 | 29.15 | 0.3421 | -1044.0 | 999999 | |
| 5.47 | -2.00 | 2.88 | -2.00 | 18.03 | 173.70 | -10.11 | 29.81 | 0.3372 | -1243.3 | 999999 | |
| 21.10 | -2.00 | 11.14 | -2.00 | 18.46 | 173.26 | -10.55 | 30.18 | 0.3468 | -1104.3 | 999999 | |
| 1.11 | -2.00 | 0.59 | -2.00 | 18.12 | 173.00 | -10.81 | 31.33 | 0.3443 | -988.0 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 18.93 | 172.56 | -11.24 | 31.06 | 0.3591 | -768.0 | -591.9 | |
| 0.00 | 6.07 | 0.00 | 3.20 | 17.69 | 172.52 | -11.29 | 33.15 | 0.3426 | -520.0 | -769.4 | |
| 0.00 | 3.08 | 0.00 | 1.62 | 18.00 | 172.50 | -11.31 | 32.68 | 0.3469 | -743.0 | -525.0 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 17.96 | 172.03 | -11.78 | 33.79 | 0.3508 | -823.0 | -657.0 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 21.11 | 171.69 | -12.12 | 29.77 | 0.3961 | -818.0 | -638.6 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 19.39 | 171.67 | -12.14 | 32.29 | 0.3730 | 677.0 | 524.1 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 17.78 | 171.78 | -12.02 | 34.64 | 0.3505 | -711.0 | -540.0 | |
| 0.00 | 1.79 | 0.00 | 0.95 | 18.33 | 171.43 | -12.38 | 34.47 | 0.3612 | 64.0 | 119.9 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 18.92 | 171.29 | -12.52 | 33.81 | 0.3702 | -903.0 | -672.4 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 18.33 | 171.24 | -12.57 | 34.88 | 0.3629 | 848.0 | 658.1 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 18.61 | 170.80 | -13.01 | 35.32 | 0.3706 | -794.0 | -666.6 | |
| 0.94 | 2.31 | 0.50 | 1.23 | 18.24 | 170.73 | -13.08 | 36.08 | 0.3665 | -964.6 | -693.4 | |
| 1.20 | 2.91 | 0.64 | 1.57 | 19.69 | 169.68 | -14.13 | 35.76 | 0.3950 | -650.5 | -652.9 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 18.70 | 169.70 | -14.11 | 37.34 | 0.3823 | 842.0 | 677.1 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 18.91 | 169.62 | -14.19 | 37.14 | 0.3858 | 661.0 | 527.8 | |
| 1.03 | 91.68 | 0.55 | 49.53 | 19.04 | 169.28 | -14.52 | 37.56 | 0.3906 | 1013.0 | 589.2 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 18.63 | 169.03 | -14.78 | 38.71 | 0.3882 | 933.0 | 754.6 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 19.78 | 168.76 | -15.05 | 37.30 | 0.4049 | 153.0 | 132.5 | |
| 2.65 | -22.00 | 1.43 | -22.00 | 19.07 | 168.76 | -15.04 | 38.46 | 0.3961 | 1170.8 | 999999 | |
| 10.25 | -22.00 | 5.54 | -22.00 | 19.13 | 168.47 | -15.34 | 38.89 | 0.3998 | 1115.2 | 999999 | |
| 3.16 | -22.00 | 1.70 | -22.00 | 18.69 | 168.47 | -15.33 | 39.61 | 0.3946 | 968.8 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.07 | 20.15 | 168.20 | -15.61 | 37.69 | 0.4149 | 970.0 | 787.6 | |
| 4.70 | -22.00 | 2.54 | -22.00 | 19.28 | 168.13 | -15.68 | 39.23 | 0.4051 | 895.1 | 999999 | |
| 0.00 | 3.25 | 0.00 | 1.77 | 20.62 | 167.99 | -15.82 | 37.32 | 0.4226 | 880.0 | 781.5 | |
| 0.34 | 1.45 | 0.19 | 0.79 | 20.31 | 167.92 | -15.88 | 37.92 | 0.4195 | 1042.0 | 871.6 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 20.78 | 167.87 | -15.93 | 37.28 | 0.4256 | 622.0 | 436.8 | |
| 2.39 | -22.00 | 1.29 | -22.00 | 18.97 | 168.03 | -15.78 | 39.93 | 0.4024 | 980.0 | 999999 | |
| 3.59 | -22.00 | 1.94 | -22.00 | 19.15 | 167.81 | -15.99 | 39.98 | 0.4068 | 923.7 | 999999 | |
| 0.00 | 3.50 | 0.00 | 1.91 | 20.18 | 167.41 | -16.40 | 38.98 | 0.4230 | 756.0 | 651.0 | |
| 0.00 | 1.88 | 0.00 | 1.03 | 19.24 | 166.56 | -17.24 | 41.90 | 0.4209 | 836.0 | 599.7 | |
| 0.00 | 1.28 | 0.00 | 0.70 | 19.99 | 166.28 | -17.53 | 41.11 | 0.4323 | 691.0 | 573.8 | |
| 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. | |