SDO HMI 2011-08-05 02:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.06 | 33.38 | 4.66 | 21.79 | 18.55 | 242.22 | -39.67 | 68.37 | 0.6526 | 106.9 | 14.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 5.43 | 0.00 | 3.36 | 18.28 | 246.22 | -35.66 | 67.38 | 0.6019 | -710.0 | -713.1 | |
| 0.00 | 0.63 | 0.00 | 0.39 | 17.53 | 246.24 | -35.65 | 68.59 | 0.5991 | -691.0 | -537.7 | |
| 0.00 | 1.18 | 0.00 | 0.73 | 17.93 | 245.55 | -36.33 | 68.21 | 0.6093 | -831.0 | -691.0 | |
| 0.00 | 2.44 | 0.00 | 1.53 | 18.03 | 245.09 | -36.79 | 68.23 | 0.6155 | -705.0 | -518.1 | |
| 3.08 | 5.70 | 1.99 | 3.68 | 18.23 | 242.88 | -39.00 | 68.68 | 0.6440 | -789.9 | -697.2 | |
| 0.00 | 1.36 | 0.00 | 0.91 | 20.00 | 240.46 | -41.42 | 66.85 | 0.6785 | 542.0 | 472.6 | |
| 0.00 | 0.54 | 0.00 | 0.36 | 18.16 | 240.81 | -41.08 | 69.42 | 0.6692 | 608.0 | 433.0 | |
| 0.90 | 2.80 | 0.61 | 1.88 | 18.96 | 240.49 | -41.40 | 68.35 | 0.6752 | 778.9 | 767.9 | |
| 0.00 | 1.54 | 0.00 | 1.03 | 19.17 | 240.42 | -41.47 | 68.06 | 0.6766 | 677.0 | 599.6 | |
| 1.27 | 2.08 | 0.84 | 1.39 | 18.21 | 240.58 | -41.31 | 69.42 | 0.6721 | 646.9 | 581.0 | |
| 0.00 | 1.45 | 0.00 | 0.97 | 18.76 | 240.33 | -41.56 | 68.69 | 0.6765 | 651.0 | 474.7 | |
| 0.00 | 0.81 | 0.00 | 0.55 | 19.30 | 239.95 | -41.94 | 68.02 | 0.6825 | 456.0 | 440.1 | |
| 1.81 | 3.44 | 1.22 | 2.32 | 18.83 | 240.01 | -41.88 | 68.67 | 0.6806 | 780.7 | 570.8 | |
| 0.00 | 2.26 | 0.00 | 1.53 | 19.01 | 239.91 | -41.98 | 68.44 | 0.6822 | 646.0 | 540.4 | |
| 0.00 | 1.72 | 0.00 | 1.16 | 18.33 | 239.55 | -42.33 | 69.53 | 0.6847 | 632.0 | 586.8 | |
| 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. | |