SDO HMI 2011-08-10 10:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.39 | 60.77 | 13.57 | 35.70 | 19.79 | 241.60 | 30.21 | 297.80 | 0.5363 | 386.5 | 76.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.63 | 3.25 | 1.03 | 2.05 | 19.12 | 248.57 | 37.18 | 292.98 | 0.6224 | -712.9 | -579.3 | |
| 0.72 | 3.43 | 0.45 | 2.15 | 19.00 | 248.01 | 36.62 | 293.00 | 0.6150 | -847.0 | -596.6 | |
| 0.00 | 7.86 | 0.00 | 4.79 | 18.39 | 245.81 | 34.42 | 292.91 | 0.5845 | -965.0 | -765.0 | |
| 0.00 | 1.26 | 0.00 | 0.77 | 18.57 | 245.38 | 33.99 | 293.40 | 0.5796 | -769.0 | -692.6 | |
| 0.00 | 1.26 | 0.00 | 0.76 | 18.42 | 244.16 | 32.77 | 293.71 | 0.5630 | -534.0 | -355.8 | |
| 1.72 | 3.07 | 1.03 | 1.83 | 18.21 | 244.07 | 32.69 | 293.39 | 0.5610 | -850.5 | -724.5 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 17.89 | 241.39 | 30.00 | 294.20 | 0.5237 | 408.0 | 379.8 | |
| 0.00 | 1.63 | 0.00 | 0.95 | 19.76 | 240.97 | 29.59 | 297.82 | 0.5274 | 746.0 | 576.1 | |
| 0.00 | 3.88 | 0.00 | 2.27 | 20.93 | 240.77 | 29.39 | 300.02 | 0.5314 | 777.0 | 741.4 | |
| 0.00 | 1.63 | 0.00 | 0.95 | 21.93 | 239.98 | 28.59 | 302.31 | 0.5273 | 854.0 | 614.8 | |
| 8.85 | 15.80 | 5.05 | 9.02 | 19.84 | 238.74 | 27.36 | 299.51 | 0.4987 | 980.4 | 821.1 | |
| 1.35 | 3.43 | 0.78 | 1.97 | 20.56 | 238.85 | 27.46 | 300.75 | 0.5044 | 619.9 | 505.8 | |
| 3.88 | -11.00 | 2.22 | -11.00 | 20.07 | 238.61 | 27.22 | 300.03 | 0.4982 | 874.9 | 999999 | |
| 5.24 | 9.75 | 3.01 | 5.60 | 21.10 | 238.73 | 27.35 | 301.81 | 0.5063 | 898.9 | 707.6 | |
| 0.00 | 3.07 | 0.00 | 1.75 | 20.84 | 238.24 | 26.85 | 301.73 | 0.4984 | 963.0 | 770.8 | |
| 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. | |