SDO HMI 2011-08-08 20:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.05 | 23.73 | 2.77 | 13.00 | -16.14 | 243.69 | 11.39 | 206.56 | 0.4279 | -12.5 | -15.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.52 | 5.78 | 1.93 | 3.16 | -14.76 | 246.26 | 13.96 | 213.26 | 0.4273 | 1049.9 | 750.2 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -15.31 | 246.24 | 13.94 | 212.48 | 0.4343 | 722.0 | 588.1 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -14.97 | 245.73 | 13.43 | 211.96 | 0.4255 | 715.0 | 591.7 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -14.68 | 245.68 | 13.38 | 212.25 | 0.4212 | 755.0 | 703.2 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -15.97 | 245.27 | 12.97 | 209.86 | 0.4353 | 943.0 | 732.8 | |
| 0.00 | 1.81 | 0.00 | 0.99 | -16.03 | 244.99 | 12.69 | 209.24 | 0.4339 | 790.0 | 611.4 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -17.32 | 242.12 | 9.82 | 202.21 | 0.4325 | -870.0 | -745.6 | |
| 0.00 | 1.26 | 0.00 | 0.70 | -18.35 | 242.08 | 9.78 | 201.22 | 0.4473 | -524.0 | -461.9 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -17.32 | 241.86 | 9.56 | 201.68 | 0.4309 | -768.0 | -627.4 | |
| 0.00 | 0.54 | 0.00 | 0.30 | -16.62 | 241.76 | 9.46 | 202.11 | 0.4202 | -755.0 | -573.7 | |
| 0.00 | 0.99 | 0.00 | 0.54 | -17.24 | 241.34 | 9.04 | 200.67 | 0.4269 | -629.0 | -563.5 | |
| 0.00 | 1.90 | 0.00 | 1.04 | -17.04 | 241.14 | 8.84 | 200.42 | 0.4227 | -898.0 | -671.9 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -17.03 | 240.46 | 8.16 | 198.99 | 0.4190 | -1020.0 | -836.3 | |
| 1.53 | 2.26 | 0.84 | 1.23 | -17.19 | 240.31 | 8.01 | 198.53 | 0.4206 | -799.0 | -713.4 | |
| 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. | |