SDO HMI 2011-08-29 06:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.36 | 0.00 | 14.34 | 16.77 | 327.96 | 5.49 | 333.13 | 0.2002 | 211.9 | 279.0 | |
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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 | 0.41 | 12.55 | 334.64 | 12.17 | 295.26 | 0.2286 | -775.0 | -622.0 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 17.12 | 334.29 | 11.82 | 311.93 | 0.2643 | -829.0 | -595.6 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 17.56 | 332.35 | 9.88 | 318.17 | 0.2463 | -786.0 | -625.2 | |
| 0.00 | 2.33 | 0.00 | 1.19 | 17.03 | 331.32 | 8.85 | 319.65 | 0.2283 | -863.0 | -635.5 | |
| 0.00 | 3.32 | 0.00 | 1.68 | 16.14 | 331.15 | 8.68 | 317.43 | 0.2153 | -772.0 | -630.9 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 17.56 | 328.56 | 6.09 | 330.88 | 0.2088 | 658.0 | 565.2 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 17.44 | 328.49 | 6.02 | 330.85 | 0.2065 | 1047.0 | 859.9 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 21.95 | 328.08 | 5.61 | 340.52 | 0.2729 | -749.0 | -541.3 | |
| 0.00 | 2.69 | 0.00 | 1.36 | 16.50 | 327.29 | 4.82 | 333.72 | 0.1828 | 717.0 | 671.6 | |
| 0.00 | 4.21 | 0.00 | 2.12 | 16.47 | 326.97 | 4.50 | 335.16 | 0.1800 | 1025.0 | 877.7 | |
| 0.00 | 1.61 | 0.00 | 0.81 | 17.18 | 326.67 | 4.20 | 338.18 | 0.1891 | 959.0 | 753.0 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 17.43 | 326.65 | 4.17 | 338.79 | 0.1929 | 845.0 | 718.0 | |
| 0.00 | 2.78 | 0.00 | 1.40 | 15.84 | 326.36 | 3.89 | 336.71 | 0.1657 | 1048.0 | 804.5 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 13.26 | 322.08 | -0.39 | 3.56 | 0.1073 | 899.0 | 704.2 | |
| 0.00 | 2.15 | 0.00 | 1.09 | 18.46 | 320.12 | -2.35 | 11.19 | 0.2011 | 755.0 | 703.5 | |
| 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. | |