SDO HMI 2011-08-24 14:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.06 | 25.25 | 1.88 | 15.55 | 7.41 | 347.53 | -36.61 | 87.06 | 0.5930 | -277.1 | -238.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.77 | 0.00 | 2.19 | 7.01 | 352.29 | -31.84 | 87.99 | 0.5260 | -999.0 | -832.4 | |
| 1.35 | 4.22 | 0.79 | 2.46 | 7.12 | 352.07 | -32.06 | 87.77 | 0.5292 | -833.3 | -826.6 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 7.11 | 351.45 | -32.68 | 87.75 | 0.5383 | -592.0 | -581.2 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 6.96 | 349.30 | -34.84 | 87.87 | 0.5696 | -568.0 | -523.7 | |
| 0.00 | 1.89 | 0.00 | 1.14 | 7.22 | 349.12 | -35.01 | 87.40 | 0.5719 | -714.0 | -537.0 | |
| 0.00 | 0.63 | 0.00 | 0.38 | 7.28 | 348.59 | -35.54 | 87.28 | 0.5794 | -486.0 | -368.9 | |
| 0.00 | 1.35 | 0.00 | 0.82 | 7.00 | 348.17 | -35.97 | 87.72 | 0.5856 | -753.0 | -593.9 | |
| 0.00 | 0.99 | 0.00 | 0.61 | 6.90 | 347.61 | -36.53 | 87.86 | 0.5935 | -644.0 | -477.5 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 7.38 | 347.45 | -36.69 | 87.05 | 0.5955 | -554.0 | -399.0 | |
| 1.71 | 2.78 | 1.09 | 1.78 | 6.57 | 344.76 | -39.37 | 88.18 | 0.6327 | -477.5 | -413.8 | |
| 0.00 | 2.96 | 0.00 | 1.90 | 7.85 | 344.35 | -39.78 | 86.14 | 0.6376 | 801.0 | 635.8 | |
| 0.00 | 0.90 | 0.00 | 0.58 | 8.01 | 343.73 | -40.40 | 85.86 | 0.6458 | 625.0 | 564.2 | |
| 0.00 | 1.26 | 0.00 | 0.82 | 8.22 | 342.93 | -41.20 | 85.51 | 0.6562 | 474.0 | 323.2 | |
| 0.00 | 1.98 | 0.00 | 1.35 | 9.26 | 340.37 | -43.77 | 83.90 | 0.6889 | 742.0 | 516.5 | |
| 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. | |