| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.53 | 37.14 | 6.51 | 20.83 | 19.74 | 125.72 | -20.75 | 45.08 | 0.4696 | 132.6 | 146.6 | |
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back to the solar disc SDO HMI 2011-12-02 11:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.03 | 141.45 | -5.02 | 14.77 | 0.3261 | 651.0 | 519.6 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.29 | 135.49 | -10.97 | 32.53 | 0.3395 | 721.0 | 515.3 | |
| 0.00 | 1.88 | 0.00 | 0.99 | 15.90 | 133.79 | -12.68 | 38.89 | 0.3378 | 944.0 | 830.2 | |
| 4.10 | 5.64 | 2.29 | 3.15 | 20.25 | 126.52 | -19.95 | 43.73 | 0.4650 | -949.9 | -807.9 | |
| 0.00 | 2.05 | 0.00 | 1.15 | 20.46 | 126.06 | -20.41 | 44.01 | 0.4722 | -697.0 | -661.6 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 20.59 | 125.84 | -20.63 | 44.11 | 0.4759 | -623.0 | -568.5 | |
| 0.00 | 3.07 | 0.00 | 1.73 | 20.65 | 125.49 | -20.98 | 44.47 | 0.4802 | -687.0 | -536.6 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 19.96 | 125.39 | -21.08 | 45.70 | 0.4744 | -720.0 | -607.3 | |
| 0.00 | 1.88 | 0.00 | 1.06 | 20.90 | 125.05 | -21.42 | 44.65 | 0.4876 | -615.0 | -480.5 | |
| 0.00 | 1.79 | 0.00 | 1.03 | 20.86 | 123.72 | -22.75 | 46.33 | 0.5016 | 798.0 | 590.8 | |
| 1.28 | 1.88 | 0.73 | 1.07 | 20.58 | 123.63 | -22.84 | 46.88 | 0.4999 | 831.8 | 763.3 | |
| 4.18 | 10.50 | 2.37 | 5.95 | 19.33 | 123.65 | -22.82 | 48.87 | 0.4879 | 954.8 | 744.2 | |
| 1.37 | 4.44 | 0.78 | 2.52 | 19.70 | 123.56 | -22.91 | 48.36 | 0.4924 | 741.8 | 599.3 | |
| 0.60 | -12.00 | 0.34 | -12.00 | 19.45 | 123.46 | -23.01 | 48.88 | 0.4912 | 854.0 | 999999 | |
| 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. | |