SDO HMI 2014-08-24 10:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.99 | 0.00 | 14.39 | -9.69 | 333.78 | 12.78 | 215.67 | 0.3713 | 237.9 | 296.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 0.91 | -9.72 | 344.25 | 23.25 | 234.45 | 0.4802 | 525.0 | 521.6 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -13.63 | 341.83 | 20.84 | 225.08 | 0.4901 | 656.0 | 514.1 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -7.62 | 339.46 | 18.47 | 231.90 | 0.4007 | 671.0 | 557.3 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -9.49 | 336.73 | 15.73 | 223.73 | 0.3884 | 757.0 | 651.8 | |
| 0.00 | 9.26 | 0.00 | 4.93 | -8.73 | 335.74 | 14.74 | 223.26 | 0.3686 | 779.0 | 684.2 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -8.16 | 335.65 | 14.66 | 224.18 | 0.3609 | 720.0 | 665.9 | |
| 0.00 | 1.80 | 0.00 | 0.95 | -8.41 | 335.57 | 14.57 | 223.53 | 0.3629 | 855.0 | 867.2 | |
| 0.00 | 1.71 | 0.00 | 0.89 | -5.91 | 333.33 | 12.33 | 223.91 | 0.3076 | 1045.0 | 899.3 | |
| 0.00 | 1.44 | 0.00 | 0.78 | -13.61 | 332.53 | 11.53 | 209.05 | 0.4018 | -578.0 | -614.4 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -13.92 | 331.97 | 10.97 | 207.49 | 0.4019 | -756.0 | -649.6 | |
| 0.00 | 0.99 | 0.00 | 0.53 | -14.08 | 331.82 | 10.82 | 206.98 | 0.4030 | -760.0 | -624.4 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -10.19 | 330.10 | 9.10 | 207.90 | 0.3342 | 782.0 | 600.2 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -13.43 | 328.54 | 7.54 | 200.13 | 0.3723 | -823.0 | -669.2 | |
| 0.00 | 2.97 | 0.00 | 1.53 | -8.95 | 319.17 | -1.83 | 173.45 | 0.2778 | -543.0 | -754.5 | |
| 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. | |