SDO HMI 2011-09-01 14:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.38 | 197.82 | 19.65 | 101.21 | 13.64 | 291.72 | 13.27 | 297.41 | 0.2528 | -712.3 | -444.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.70 | 0.00 | 0.88 | 13.77 | 293.79 | 15.34 | 294.86 | 0.2845 | -715.0 | -523.6 | |
| 0.00 | 1.61 | 0.00 | 0.84 | 18.47 | 293.67 | 15.22 | 308.74 | 0.3207 | 743.0 | 629.4 | |
| 0.00 | 1.25 | 0.00 | 0.65 | 14.91 | 293.32 | 14.87 | 299.19 | 0.2854 | -817.0 | -637.6 | |
| 0.00 | 1.16 | 0.00 | 0.61 | 18.41 | 293.50 | 15.05 | 308.89 | 0.3180 | 860.0 | 666.1 | |
| 0.00 | 1.79 | 0.00 | 0.92 | 13.47 | 292.54 | 14.10 | 295.55 | 0.2638 | -840.0 | -581.1 | |
| 6.89 | 182.43 | 3.53 | 93.30 | 13.25 | 291.96 | 13.51 | 295.61 | 0.2533 | -1097.1 | -493.0 | |
| 1.52 | -6.00 | 0.78 | -6.00 | 12.97 | 291.91 | 13.46 | 294.68 | 0.2508 | -929.2 | 999999 | |
| 6.26 | -6.00 | 3.21 | -6.00 | 14.01 | 291.87 | 13.43 | 298.48 | 0.2575 | -1122.8 | 999999 | |
| 23.71 | -6.00 | 12.13 | -6.00 | 13.44 | 291.65 | 13.20 | 296.79 | 0.2500 | -1213.4 | 999999 | |
| 0.00 | 3.49 | 0.00 | 1.78 | 13.64 | 291.02 | 12.57 | 298.60 | 0.2421 | -878.0 | -568.2 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 19.97 | 291.03 | 12.58 | 317.58 | 0.3049 | 870.0 | 675.6 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 16.17 | 288.82 | 10.38 | 312.41 | 0.2354 | 698.0 | 524.3 | |
| 0.00 | 1.97 | 0.00 | 1.00 | 15.95 | 287.09 | 8.65 | 316.79 | 0.2121 | 1015.0 | 759.6 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 16.57 | 286.74 | 8.29 | 319.95 | 0.2158 | 864.0 | 704.9 | |
| 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. | |