SDO HMI 2011-06-03 08:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.85 | 35.02 | 5.78 | 18.44 | 17.07 | 40.96 | 8.66 | 335.35 | 0.3397 | -179.7 | -30.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.32 | 12.48 | 4.46 | 6.69 | 18.08 | 45.52 | 13.22 | 325.58 | 0.3862 | -1042.2 | -770.3 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 12.46 | 43.54 | 11.24 | 319.49 | 0.2942 | -815.0 | -643.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 16.17 | 42.89 | 10.59 | 328.26 | 0.3370 | -885.0 | -707.9 | |
| 0.72 | 2.35 | 0.38 | 1.24 | 16.96 | 41.55 | 9.25 | 332.77 | 0.3373 | -1002.6 | -795.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 16.67 | 41.50 | 9.20 | 332.47 | 0.3328 | -864.0 | -694.8 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 16.32 | 41.03 | 8.73 | 333.16 | 0.3242 | -886.0 | -628.6 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 15.09 | 40.02 | 7.73 | 334.10 | 0.2984 | -743.0 | -535.5 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 16.76 | 37.34 | 5.04 | 344.10 | 0.3085 | 844.0 | 661.4 | |
| 1.81 | 2.35 | 0.94 | 1.22 | 16.54 | 37.14 | 4.85 | 344.48 | 0.3041 | 805.2 | 603.0 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 16.48 | 36.89 | 4.59 | 345.21 | 0.3019 | 895.0 | 746.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.25 | 36.18 | 3.89 | 347.22 | 0.2955 | 961.0 | 742.2 | |
| 0.00 | 2.53 | 0.00 | 1.32 | 16.70 | 35.78 | 3.48 | 348.82 | 0.3014 | 670.0 | 665.4 | |
| 0.00 | 2.26 | 0.00 | 1.17 | 16.29 | 35.71 | 3.41 | 348.76 | 0.2944 | 960.0 | 749.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 17.40 | 35.12 | 2.82 | 351.26 | 0.3110 | 916.0 | 755.9 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 19.30 | 35.12 | 2.82 | 352.15 | 0.3420 | 847.0 | 573.5 | |
| 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. | |