| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.74 | 199.74 | 16.84 | 106.61 | 19.59 | 103.59 | -10.45 | 27.49 | 0.3718 | -692.7 | -354.2 | |
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back to the solar disc SDO HMI 2011-12-04 22:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.33 | 0.00 | 1.83 | 24.62 | 104.73 | -9.32 | 19.77 | 0.4371 | -704.0 | -623.8 | |
| 0.00 | 1.71 | 0.00 | 0.93 | 22.47 | 104.10 | -9.94 | 23.05 | 0.4094 | -1019.0 | -726.2 | |
| 31.74 | 175.83 | 16.84 | 93.33 | 19.03 | 104.04 | -10.00 | 27.25 | 0.3602 | -1275.6 | -401.7 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 22.63 | 103.60 | -10.44 | 23.90 | 0.4148 | -873.0 | -628.4 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 28.04 | 102.60 | -11.44 | 20.70 | 0.4973 | -757.0 | -564.5 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 25.21 | 102.42 | -11.62 | 23.52 | 0.4588 | -653.0 | -592.1 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 26.28 | 101.94 | -12.10 | 23.32 | 0.4767 | -712.0 | -577.0 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 26.22 | 101.72 | -12.33 | 23.77 | 0.4772 | -768.0 | -698.0 | |
| 0.00 | 1.37 | 0.00 | 0.80 | 29.89 | 100.54 | -13.50 | 22.38 | 0.5339 | -697.0 | -549.7 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 15.85 | 101.34 | -12.71 | 38.53 | 0.3412 | 850.0 | 660.7 | |
| 0.00 | 2.56 | 0.00 | 1.51 | 30.33 | 99.10 | -14.94 | 24.06 | 0.5480 | -466.0 | -479.1 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 17.60 | 100.07 | -13.97 | 37.95 | 0.3759 | 762.0 | 697.5 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 18.44 | 99.07 | -14.98 | 38.42 | 0.3962 | 773.0 | 574.4 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 18.31 | 98.76 | -15.29 | 39.19 | 0.3978 | 722.0 | 581.8 | |
| 0.00 | 3.16 | 0.00 | 1.78 | 23.00 | 95.65 | -18.40 | 37.12 | 0.4835 | 753.0 | 697.7 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 19.21 | 95.93 | -18.12 | 42.36 | 0.4376 | 717.0 | 556.8 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 19.36 | 95.71 | -18.33 | 42.43 | 0.4416 | 805.0 | 683.6 | |
| 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. | |