SDO HMI 2011-07-04 23:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.69 | 125.22 | 23.80 | 104.39 | 15.44 | 26.73 | 53.05 | 286.84 | 0.8067 | -367.6 | -271.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 1.21 | 16.97 | 29.12 | 55.44 | 288.31 | 0.8318 | -378.0 | -295.7 | |
| 14.99 | 93.54 | 12.71 | 79.06 | 15.34 | 27.46 | 53.78 | 286.59 | 0.8139 | -795.0 | -417.2 | |
| 0.00 | 0.45 | 0.00 | 0.39 | 17.24 | 28.18 | 54.49 | 288.78 | 0.8233 | -539.0 | -545.8 | |
| 3.72 | -2.00 | 3.13 | -2.00 | 14.95 | 27.05 | 53.37 | 286.17 | 0.8094 | -799.2 | 999999 | |
| 0.00 | 1.27 | 0.00 | 1.08 | 16.22 | 27.48 | 53.80 | 287.66 | 0.8153 | -449.0 | -373.5 | |
| 0.00 | 1.09 | 0.00 | 0.89 | 15.60 | 25.97 | 52.28 | 287.14 | 0.7995 | -618.0 | -535.2 | |
| 1.45 | 3.63 | 1.19 | 2.97 | 15.41 | 25.85 | 52.17 | 286.93 | 0.7981 | -352.8 | 88.0 | |
| 1.45 | -7.00 | 1.19 | -7.00 | 15.36 | 25.72 | 52.04 | 286.88 | 0.7967 | 165.0 | 999999 | |
| 0.00 | 2.36 | 0.00 | 1.87 | 16.27 | 24.27 | 50.58 | 288.29 | 0.7833 | 160.0 | 71.6 | |
| 3.09 | 14.62 | 2.43 | 11.49 | 15.78 | 23.99 | 50.31 | 287.72 | 0.7796 | 449.6 | 492.2 | |
| 2.72 | 4.27 | 2.15 | 3.37 | 16.66 | 23.96 | 50.27 | 288.84 | 0.7808 | 542.7 | 516.0 | |
| 1.27 | 1.45 | 1.00 | 1.14 | 16.42 | 23.77 | 50.08 | 288.57 | 0.7784 | 706.1 | 613.0 | |
| 0.00 | 1.18 | 0.00 | 0.92 | 15.74 | 23.34 | 49.65 | 287.80 | 0.7727 | 734.0 | 638.0 | |
| 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. | |