SDO HMI 2011-08-09 07:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.53 | 23.76 | 0.87 | 13.43 | -16.34 | 244.03 | 17.77 | 217.67 | 0.4840 | 100.3 | 8.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.67 | -14.47 | 246.85 | 20.59 | 224.38 | 0.4888 | 648.0 | 517.7 | |
| 1.17 | 2.53 | 0.67 | 1.43 | -14.56 | 246.65 | 20.40 | 223.98 | 0.4878 | 919.0 | 762.7 | |
| 0.00 | 2.89 | 0.00 | 1.64 | -15.09 | 246.20 | 19.95 | 222.57 | 0.4889 | 883.0 | 777.3 | |
| 0.36 | 1.99 | 0.20 | 1.12 | -14.63 | 245.96 | 19.70 | 222.89 | 0.4812 | 973.2 | 835.3 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -15.08 | 245.93 | 19.68 | 222.20 | 0.4860 | 728.0 | 604.0 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -15.21 | 245.81 | 19.56 | 221.84 | 0.4862 | 475.0 | 380.5 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -15.23 | 245.58 | 19.33 | 221.47 | 0.4841 | 269.0 | 294.3 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -15.76 | 244.93 | 18.68 | 219.77 | 0.4837 | 908.0 | 794.0 | |
| 0.00 | 1.81 | 0.00 | 1.02 | -17.39 | 242.39 | 16.13 | 213.68 | 0.4801 | -865.0 | -749.0 | |
| 0.00 | 1.81 | 0.00 | 1.02 | -17.78 | 242.09 | 15.84 | 212.74 | 0.4825 | -701.0 | -628.5 | |
| 0.00 | 2.53 | 0.00 | 1.42 | -17.30 | 241.52 | 15.26 | 212.36 | 0.4716 | -960.0 | -817.7 | |
| 0.00 | 2.17 | 0.00 | 1.21 | -17.06 | 241.37 | 15.11 | 212.38 | 0.4673 | -792.0 | -729.0 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -16.86 | 241.22 | 14.96 | 212.37 | 0.4635 | -446.0 | -485.4 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -24.16 | 240.35 | 14.10 | 203.79 | 0.5530 | -540.0 | -453.1 | |
| 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. | |