SDO HMI 2014-07-07 17:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.72 | 37.70 | 2.49 | 19.92 | 7.60 | 252.21 | 20.25 | 282.23 | 0.3526 | 381.6 | 458.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.63 | 7.39 | 254.38 | 22.42 | 280.70 | 0.3866 | -747.0 | -592.2 | |
| 0.45 | 2.91 | 0.24 | 1.56 | 7.27 | 254.14 | 22.18 | 280.49 | 0.3825 | -893.2 | -686.6 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 7.04 | 253.67 | 21.71 | 280.06 | 0.3744 | -845.0 | -720.6 | |
| 0.00 | 2.18 | 0.00 | 1.16 | 6.98 | 253.50 | 21.54 | 279.97 | 0.3716 | -963.0 | -790.7 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 8.00 | 253.16 | 21.20 | 282.84 | 0.3688 | 829.0 | 600.9 | |
| 1.91 | 8.26 | 1.01 | 4.38 | 8.17 | 252.34 | 20.38 | 283.74 | 0.3564 | 939.0 | 734.3 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 7.32 | 252.10 | 20.14 | 281.49 | 0.3500 | 697.0 | 519.6 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 7.84 | 252.13 | 20.17 | 282.94 | 0.3519 | 634.0 | 482.1 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 8.64 | 252.04 | 20.08 | 285.21 | 0.3533 | 795.0 | 708.3 | |
| 0.00 | 2.18 | 0.00 | 1.15 | 8.52 | 251.90 | 19.94 | 284.96 | 0.3506 | 1033.0 | 870.3 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 7.91 | 251.87 | 19.91 | 283.27 | 0.3480 | 815.0 | 696.7 | |
| 0.00 | 1.73 | 0.00 | 0.91 | 8.15 | 251.82 | 19.86 | 283.99 | 0.3480 | 996.0 | 801.1 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 7.55 | 251.52 | 19.56 | 282.43 | 0.3414 | 685.0 | 544.1 | |
| 2.36 | 9.81 | 1.24 | 5.16 | 7.22 | 251.31 | 19.35 | 281.57 | 0.3370 | 1017.6 | 886.9 | |
| 0.00 | 2.00 | 0.00 | 1.04 | 6.35 | 250.50 | 18.54 | 279.33 | 0.3216 | 879.0 | 789.0 | |
| 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. | |