SDO HMI 2011-08-11 03:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.22 | 22.91 | 4.53 | 14.76 | 20.29 | 240.19 | 38.19 | 294.48 | 0.6389 | 407.4 | 184.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.08 | 0.00 | 1.46 | 18.43 | 246.56 | 44.56 | 289.71 | 0.7094 | -646.0 | -519.6 | |
| 0.00 | 1.17 | 0.00 | 0.81 | 17.33 | 246.17 | 44.16 | 288.25 | 0.7026 | -724.0 | -618.8 | |
| 0.00 | 1.26 | 0.00 | 0.86 | 18.49 | 244.49 | 42.49 | 290.29 | 0.6853 | -612.0 | -470.1 | |
| 0.00 | 1.90 | 0.00 | 1.23 | 21.52 | 240.37 | 38.36 | 296.11 | 0.6452 | 720.0 | 573.0 | |
| 4.60 | 6.59 | 2.89 | 4.14 | 19.52 | 238.64 | 36.64 | 293.74 | 0.6167 | 858.4 | 639.1 | |
| 0.00 | 0.99 | 0.00 | 0.64 | 23.26 | 239.76 | 37.75 | 298.95 | 0.6451 | 457.0 | 330.6 | |
| 0.00 | 1.17 | 0.00 | 0.74 | 20.62 | 238.74 | 36.73 | 295.41 | 0.6220 | 632.0 | 475.3 | |
| 0.00 | 0.99 | 0.00 | 0.63 | 20.88 | 238.57 | 36.57 | 295.89 | 0.6210 | 465.0 | 336.2 | |
| 0.00 | 0.72 | 0.00 | 0.46 | 23.02 | 239.01 | 37.01 | 298.94 | 0.6353 | 470.0 | 453.8 | |
| 2.62 | 2.89 | 1.64 | 1.81 | 20.74 | 238.29 | 36.28 | 295.80 | 0.6169 | 771.7 | 485.5 | |
| 0.00 | 0.99 | 0.00 | 0.63 | 23.06 | 238.86 | 36.85 | 299.07 | 0.6337 | 576.0 | 522.5 | |
| 0.00 | 1.08 | 0.00 | 0.68 | 20.60 | 237.97 | 35.96 | 295.73 | 0.6124 | 661.0 | 523.6 | |
| 0.00 | 1.08 | 0.00 | 0.67 | 23.05 | 235.89 | 33.89 | 300.62 | 0.5984 | 582.0 | 444.4 | |
| 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. | |