SDO HMI 2011-08-04 23:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.49 | 32.19 | 7.53 | 21.56 | 18.51 | 242.14 | -41.40 | 68.96 | 0.6735 | -134.5 | 317.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.80 | 4.97 | 2.40 | 3.14 | 18.23 | 246.18 | -37.36 | 68.10 | 0.6234 | -855.4 | -656.2 | |
| 0.00 | 1.45 | 0.00 | 0.92 | 17.87 | 245.91 | -37.63 | 68.76 | 0.6257 | -780.0 | -602.1 | |
| 0.00 | 1.18 | 0.00 | 0.75 | 17.57 | 245.74 | -37.80 | 69.28 | 0.6269 | -660.0 | -531.7 | |
| 0.00 | 0.90 | 0.00 | 0.58 | 17.90 | 245.45 | -38.08 | 68.87 | 0.6315 | -785.0 | -651.8 | |
| 5.61 | 5.61 | 3.71 | 3.71 | 18.36 | 242.84 | -40.70 | 69.00 | 0.6652 | -751.0 | -734.0 | |
| 0.00 | 1.36 | 0.00 | 0.93 | 19.18 | 240.55 | -42.98 | 68.47 | 0.6945 | 571.0 | 545.3 | |
| 0.00 | 5.06 | 0.00 | 3.47 | 18.87 | 240.61 | -42.93 | 68.90 | 0.6931 | 717.0 | 677.6 | |
| 2.08 | 2.35 | 1.42 | 1.60 | 18.19 | 240.78 | -42.76 | 69.82 | 0.6895 | 719.5 | 638.0 | |
| 0.00 | 0.81 | 0.00 | 0.56 | 18.46 | 240.61 | -42.93 | 69.48 | 0.6921 | 562.0 | 457.8 | |
| 0.00 | 1.27 | 0.00 | 0.88 | 19.20 | 240.01 | -43.52 | 68.58 | 0.7009 | 512.0 | 414.6 | |
| 0.00 | 5.33 | 0.00 | 3.69 | 18.86 | 239.99 | -43.54 | 69.08 | 0.7003 | 557.0 | 605.6 | |
| 0.00 | 0.63 | 0.00 | 0.44 | 18.45 | 239.63 | -43.90 | 69.73 | 0.7035 | 255.0 | 323.6 | |
| 0.00 | 1.27 | 0.00 | 0.89 | 18.26 | 239.16 | -44.38 | 70.11 | 0.7086 | 510.0 | 331.6 | |
| 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. | |