SDO HMI 2011-10-05 14:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.43 | 197.33 | 20.95 | 104.67 | -11.62 | 178.97 | -10.63 | 149.77 | 0.3598 | 508.7 | 373.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.84 | 178.11 | 0.98 | 94.29 | -11.90 | 179.49 | -10.11 | 151.31 | 0.3593 | 724.0 | 461.9 | |
| 1.14 | -1.00 | 0.61 | -1.00 | -11.90 | 179.37 | -10.24 | 151.01 | 0.3603 | 648.0 | 999999 | |
| 30.83 | -1.00 | 16.32 | -1.00 | -11.49 | 179.32 | -10.28 | 150.33 | 0.3549 | 1235.0 | 999999 | |
| 1.41 | -1.00 | 0.75 | -1.00 | -11.79 | 178.72 | -10.88 | 149.33 | 0.3640 | 651.9 | 999999 | |
| 0.53 | 3.95 | 0.28 | 2.11 | -11.98 | 178.49 | -11.11 | 149.09 | 0.3686 | 792.0 | 575.8 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -12.43 | 177.12 | -12.48 | 146.74 | 0.3864 | -700.0 | -595.7 | |
| 0.00 | 2.28 | 0.00 | 1.23 | -12.47 | 176.84 | -12.76 | 146.20 | 0.3894 | -938.0 | -829.0 | |
| 0.70 | 3.95 | 0.38 | 2.13 | -12.69 | 176.57 | -13.03 | 145.99 | 0.3948 | -993.9 | -805.5 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -13.14 | 176.49 | -13.11 | 146.45 | 0.4015 | -765.0 | -522.6 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -12.10 | 174.17 | -15.43 | 140.44 | 0.4102 | -754.0 | -593.6 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -12.33 | 173.87 | -15.73 | 140.26 | 0.4161 | -908.0 | -777.5 | |
| 2.37 | 3.07 | 1.29 | 1.67 | -12.21 | 173.62 | -15.98 | 139.63 | 0.4172 | -934.3 | -645.0 | |
| 0.61 | 2.37 | 0.34 | 1.29 | -12.59 | 173.53 | -16.07 | 140.07 | 0.4227 | -1039.6 | -845.3 | |
| 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. | |