| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.37 | 181.24 | 26.65 | 113.72 | 18.35 | 103.22 | 33.63 | 300.94 | 0.6151 | -83.3 | -241.5 | |
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back to the solar disc SDO HMI 2011-12-08 07:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.71 | 23.87 | 10.59 | 15.13 | 17.07 | 104.71 | 35.12 | 298.10 | 0.6258 | 877.7 | 594.0 | |
| 0.51 | -1.00 | 0.32 | -1.00 | 17.44 | 104.56 | 34.98 | 298.73 | 0.6260 | 778.3 | 999999 | |
| 0.00 | 2.81 | 0.00 | 1.75 | 16.76 | 103.44 | 33.86 | 298.40 | 0.6087 | 543.0 | 467.8 | |
| 0.00 | 0.85 | 0.00 | 0.53 | 17.25 | 103.17 | 33.59 | 299.32 | 0.6082 | -529.0 | -437.7 | |
| 18.33 | 126.36 | 11.55 | 79.67 | 18.78 | 103.43 | 33.84 | 301.41 | 0.6201 | -1180.7 | -346.9 | |
| 3.33 | 10.40 | 2.04 | 6.40 | 17.75 | 101.83 | 32.25 | 300.97 | 0.5949 | -973.5 | -548.8 | |
| 2.13 | 6.31 | 1.31 | 3.87 | 18.28 | 101.28 | 31.69 | 302.16 | 0.5916 | -914.3 | -175.9 | |
| 1.36 | 2.30 | 0.84 | 1.42 | 19.15 | 101.28 | 31.69 | 303.47 | 0.5972 | -793.2 | -748.8 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 16.17 | 99.87 | 30.29 | 299.91 | 0.5610 | 695.0 | 564.1 | |
| 0.00 | 1.19 | 0.00 | 0.71 | 16.14 | 99.62 | 30.03 | 300.05 | 0.5576 | 622.0 | 558.1 | |
| 0.00 | 2.47 | 0.00 | 1.47 | 16.66 | 99.25 | 29.66 | 301.18 | 0.5563 | 700.0 | 534.2 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 14.88 | 98.64 | 29.06 | 298.70 | 0.5373 | 569.0 | 377.6 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 16.35 | 98.52 | 28.94 | 301.25 | 0.5452 | 827.0 | 719.3 | |
| 0.00 | 1.28 | 0.00 | 0.76 | 18.90 | 98.40 | 28.82 | 305.39 | 0.5616 | 769.0 | 634.7 | |
| 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. | |