SDO HMI 2011-08-04 16:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.54 | 37.60 | 12.25 | 26.06 | 18.14 | 243.64 | -43.77 | 70.09 | 0.7009 | -275.5 | -260.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.54 | 17.51 | 246.70 | -40.71 | 70.22 | 0.6633 | -519.0 | -463.9 | |
| 7.05 | 7.96 | 4.72 | 5.32 | 18.12 | 245.89 | -41.52 | 69.56 | 0.6747 | -794.5 | -688.8 | |
| 0.00 | 1.63 | 0.00 | 1.09 | 17.46 | 245.90 | -41.51 | 70.51 | 0.6729 | -703.0 | -591.9 | |
| 0.00 | 2.17 | 0.00 | 1.45 | 17.82 | 245.71 | -41.70 | 70.03 | 0.6760 | -769.0 | -648.9 | |
| 0.00 | 1.36 | 0.00 | 0.91 | 17.77 | 245.43 | -41.98 | 70.18 | 0.6794 | -752.0 | -617.7 | |
| 0.00 | 2.98 | 0.00 | 2.01 | 17.55 | 245.45 | -41.96 | 70.49 | 0.6786 | -655.0 | -518.2 | |
| 0.00 | 0.90 | 0.00 | 0.61 | 17.07 | 245.28 | -42.13 | 71.23 | 0.6795 | -670.0 | -419.4 | |
| 0.00 | 1.18 | 0.00 | 0.80 | 18.15 | 244.49 | -42.92 | 69.89 | 0.6914 | -516.0 | -389.8 | |
| 0.00 | 0.99 | 0.00 | 0.68 | 17.94 | 244.25 | -43.16 | 70.24 | 0.6939 | -310.0 | -308.7 | |
| 4.34 | 7.23 | 3.05 | 5.08 | 18.37 | 242.77 | -44.64 | 69.99 | 0.7120 | -554.9 | -326.9 | |
| 0.00 | 2.08 | 0.00 | 1.51 | 18.65 | 241.02 | -46.39 | 69.99 | 0.7324 | 698.0 | 544.7 | |
| 0.00 | 0.45 | 0.00 | 0.33 | 19.01 | 240.75 | -46.66 | 69.57 | 0.7361 | 650.0 | 634.4 | |
| 3.71 | 4.97 | 2.68 | 3.60 | 18.15 | 240.97 | -46.44 | 70.69 | 0.7320 | 676.5 | 546.3 | |
| 2.44 | 2.89 | 1.80 | 2.13 | 18.91 | 240.17 | -47.24 | 69.83 | 0.7422 | 581.1 | 513.4 | |
| 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. | |