SDO HMI 2014-08-13 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.24 | 371.40 | 35.00 | 211.91 | 15.11 | 133.69 | 28.96 | 289.16 | 0.4969 | -855.6 | -344.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.52 | 355.02 | 34.62 | 203.13 | 15.24 | 134.01 | 29.28 | 289.29 | 0.5020 | -1360.0 | -386.0 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 18.46 | 129.31 | 24.58 | 298.72 | 0.4517 | -781.0 | -710.5 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 11.71 | 127.23 | 22.50 | 284.73 | 0.3891 | -839.0 | -647.8 | |
| 0.00 | 1.80 | 0.00 | 0.97 | 12.81 | 127.33 | 22.60 | 287.42 | 0.3944 | 615.0 | 539.8 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 12.11 | 127.10 | 22.37 | 285.82 | 0.3884 | 749.0 | 628.8 | |
| 0.00 | 1.62 | 0.00 | 0.87 | 12.42 | 127.09 | 22.36 | 286.59 | 0.3894 | 936.0 | 750.2 | |
| 0.00 | 1.80 | 0.00 | 0.97 | 12.70 | 126.98 | 22.25 | 287.36 | 0.3887 | 753.0 | 692.5 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 10.53 | 126.17 | 21.44 | 282.14 | 0.3691 | 800.0 | 600.5 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 11.94 | 126.14 | 21.42 | 285.89 | 0.3730 | 807.0 | 618.9 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 11.76 | 126.06 | 21.33 | 285.46 | 0.3711 | 837.0 | 670.3 | |
| 0.72 | 1.80 | 0.38 | 0.96 | 10.64 | 125.74 | 21.01 | 282.62 | 0.3627 | 887.5 | 741.2 | |
| 0.00 | 1.53 | 0.00 | 0.81 | 10.27 | 124.37 | 19.64 | 282.20 | 0.3398 | 1031.0 | 859.7 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 12.62 | 123.65 | 18.92 | 289.46 | 0.3370 | 738.0 | 591.7 | |
| 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. | |