| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89.07 | 226.16 | 46.98 | 119.25 | 19.01 | 170.70 | -8.69 | 24.37 | 0.3429 | 29.4 | 11.8 | |
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back to the solar disc SDO HMI 2011-11-29 23:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.14 | 0.00 | 1.12 | 19.31 | 175.20 | -4.19 | 12.42 | 0.3219 | -843.0 | -651.4 | |
| 0.51 | 84.35 | 0.27 | 44.01 | 18.57 | 173.94 | -5.45 | 16.68 | 0.3152 | 103.7 | -463.7 | |
| 3.85 | -2.00 | 2.00 | -2.00 | 18.04 | 173.86 | -5.53 | 17.43 | 0.3073 | -1225.5 | 999999 | |
| 31.88 | -2.00 | 16.62 | -2.00 | 18.41 | 173.69 | -5.70 | 17.54 | 0.3140 | -1085.2 | 999999 | |
| 0.26 | -2.00 | 0.13 | -2.00 | 18.66 | 173.24 | -6.14 | 18.55 | 0.3202 | -779.7 | 999999 | |
| 0.00 | 2.99 | 0.00 | 1.56 | 18.63 | 172.81 | -6.58 | 19.81 | 0.3221 | -512.0 | -584.0 | |
| 0.00 | 5.56 | 0.00 | 2.89 | 17.98 | 172.77 | -6.62 | 20.66 | 0.3122 | -946.0 | -797.0 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.35 | 172.75 | -6.63 | 20.27 | 0.3180 | -687.0 | -538.3 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 20.68 | 171.70 | -7.69 | 20.44 | 0.3599 | -759.0 | -499.5 | |
| 0.00 | 9.32 | 0.00 | 4.89 | 18.93 | 171.60 | -7.79 | 22.68 | 0.3340 | -1087.0 | -795.1 | |
| 1.37 | 3.76 | 0.72 | 1.97 | 18.22 | 171.09 | -8.29 | 24.92 | 0.3267 | 957.8 | 764.0 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 18.62 | 170.79 | -8.60 | 25.15 | 0.3347 | -750.0 | -530.1 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 19.93 | 170.05 | -9.33 | 25.25 | 0.3591 | -1002.0 | -693.8 | |
| 2.48 | 3.85 | 1.31 | 2.04 | 19.90 | 169.83 | -9.56 | 25.81 | 0.3602 | -792.6 | -665.1 | |
| 0.00 | 8.89 | 0.00 | 4.70 | 19.11 | 169.34 | -10.05 | 28.01 | 0.3526 | 439.0 | 867.0 | |
| 2.82 | 3.85 | 1.49 | 2.04 | 18.80 | 168.56 | -10.82 | 30.26 | 0.3544 | 1001.9 | 747.5 | |
| 1.71 | 65.12 | 0.91 | 34.61 | 19.45 | 168.46 | -10.93 | 29.53 | 0.3643 | 831.0 | 564.8 | |
| 18.37 | -17.00 | 9.76 | -17.00 | 19.27 | 168.44 | -10.95 | 29.85 | 0.3619 | 1124.8 | 999999 | |
| 0.00 | 2.65 | 0.00 | 1.42 | 20.77 | 168.27 | -11.12 | 28.14 | 0.3841 | 1039.0 | 758.1 | |
| 8.38 | -17.00 | 4.46 | -17.00 | 19.42 | 167.95 | -11.44 | 30.70 | 0.3680 | 844.7 | 999999 | |
| 4.79 | 23.08 | 2.57 | 12.36 | 20.52 | 167.83 | -11.55 | 29.38 | 0.3840 | 866.9 | 706.7 | |
| 3.25 | -21.00 | 1.74 | -21.00 | 20.20 | 167.76 | -11.63 | 29.97 | 0.3803 | 1015.4 | 999999 | |
| 9.40 | -17.00 | 5.00 | -17.00 | 19.05 | 167.69 | -11.70 | 31.82 | 0.3651 | 945.0 | 999999 | |
| 0.00 | 2.31 | 0.00 | 1.23 | 19.48 | 167.62 | -11.76 | 31.30 | 0.3716 | 456.0 | 339.9 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 19.98 | 167.10 | -12.28 | 31.65 | 0.3827 | 745.0 | 480.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 19.51 | 166.53 | -12.86 | 33.52 | 0.3815 | 683.0 | 595.4 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 19.26 | 166.36 | -13.03 | 34.26 | 0.3798 | 948.0 | 722.7 | |
| 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. | |