SDO HMI 2011-08-25 10:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.35 | 25.45 | 0.74 | 14.38 | 9.03 | 344.71 | -28.42 | 84.94 | 0.4719 | -383.3 | -361.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.98 | 0.00 | 1.05 | 5.85 | 352.43 | -20.70 | 92.08 | 0.3533 | -885.0 | -714.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 7.02 | 352.18 | -20.94 | 88.73 | 0.3564 | -824.0 | -747.7 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 6.56 | 351.48 | -21.64 | 89.93 | 0.3680 | -802.0 | -617.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 7.73 | 351.23 | -21.90 | 86.73 | 0.3718 | -656.0 | -592.0 | |
| 0.00 | 1.80 | 0.00 | 0.96 | 7.31 | 351.25 | -21.88 | 87.88 | 0.3714 | -703.0 | -563.9 | |
| 0.00 | 2.69 | 0.00 | 1.45 | 7.11 | 350.27 | -22.86 | 88.36 | 0.3872 | -912.0 | -732.0 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 7.37 | 348.15 | -24.98 | 87.62 | 0.4209 | -623.0 | -552.0 | |
| 0.00 | 1.80 | 0.00 | 0.98 | 7.06 | 348.03 | -25.10 | 88.35 | 0.4229 | -605.0 | -504.7 | |
| 1.35 | 1.71 | 0.74 | 0.93 | 6.59 | 347.75 | -25.37 | 89.44 | 0.4275 | -791.7 | -794.8 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 9.11 | 344.93 | -28.19 | 83.79 | 0.4711 | 673.0 | 523.5 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 7.02 | 345.02 | -28.10 | 88.26 | 0.4696 | -648.0 | -507.2 | |
| 0.00 | 1.26 | 0.00 | 0.71 | 8.29 | 343.81 | -29.31 | 85.57 | 0.4879 | 796.0 | 623.4 | |
| 0.00 | 1.62 | 0.00 | 0.96 | 10.30 | 339.13 | -34.00 | 81.96 | 0.5578 | 714.0 | 581.2 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 10.79 | 338.69 | -34.44 | 81.13 | 0.5644 | 674.0 | 598.2 | |
| 0.00 | 2.87 | 0.00 | 1.80 | 13.76 | 335.17 | -37.95 | 76.60 | 0.6163 | -778.0 | -687.8 | |
| 0.00 | 1.08 | 0.00 | 0.69 | 14.29 | 333.62 | -39.51 | 76.02 | 0.6376 | -697.0 | -539.7 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 14.28 | 333.09 | -40.03 | 76.13 | 0.6444 | -555.0 | -403.0 | |
| 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. | |