SDO HMI 2014-08-16 06:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.18 | 313.42 | 66.78 | 220.70 | 16.18 | 23.69 | -45.22 | 73.72 | 0.7111 | -40.0 | -91.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.48 | 17.79 | 27.96 | -40.96 | 70.61 | 0.6639 | 506.0 | 421.5 | |
| 20.73 | 140.09 | 13.75 | 92.96 | 16.17 | 27.46 | -41.45 | 73.15 | 0.6666 | -1090.7 | -428.4 | |
| 1.53 | -2.00 | 1.02 | -2.00 | 16.65 | 27.21 | -41.71 | 72.49 | 0.6707 | -869.9 | 999999 | |
| 12.53 | -2.00 | 8.40 | -2.00 | 16.80 | 26.83 | -42.09 | 72.34 | 0.6757 | -749.1 | 999999 | |
| 0.00 | 1.62 | 0.00 | 1.10 | 16.64 | 26.31 | -42.60 | 72.69 | 0.6817 | -664.0 | -500.3 | |
| 0.00 | 1.35 | 0.00 | 0.92 | 16.68 | 26.04 | -42.88 | 72.68 | 0.6850 | -554.0 | -429.9 | |
| 5.50 | 15.96 | 3.73 | 10.83 | 16.06 | 25.99 | -42.92 | 73.60 | 0.6845 | -893.0 | -437.4 | |
| 6.49 | -7.00 | 4.41 | -7.00 | 16.24 | 25.90 | -43.01 | 73.35 | 0.6859 | -759.0 | 999999 | |
| 2.70 | 7.66 | 1.85 | 5.23 | 16.81 | 25.66 | -43.26 | 72.57 | 0.6899 | -683.9 | -229.7 | |
| 0.00 | 0.99 | 0.00 | 0.67 | 15.42 | 25.73 | -43.19 | 74.57 | 0.6867 | -671.0 | -573.5 | |
| 0.00 | 1.44 | 0.00 | 0.99 | 15.79 | 25.41 | -43.50 | 74.08 | 0.6911 | -354.0 | -323.4 | |
| 0.00 | 0.63 | 0.00 | 0.43 | 15.58 | 25.42 | -43.49 | 74.39 | 0.6906 | -367.0 | -313.9 | |
| 0.00 | 0.81 | 0.00 | 0.56 | 16.95 | 25.00 | -43.91 | 72.51 | 0.6979 | -395.0 | -369.0 | |
| 0.00 | 1.17 | 0.00 | 0.80 | 15.24 | 25.43 | -43.49 | 74.88 | 0.6901 | -562.0 | -475.5 | |
| 0.00 | 1.89 | 0.00 | 1.30 | 15.99 | 25.10 | -43.82 | 73.86 | 0.6952 | -116.0 | -221.5 | |
| 0.00 | 0.90 | 0.00 | 0.62 | 14.98 | 25.36 | -43.55 | 75.26 | 0.6906 | -584.0 | -473.1 | |
| 0.00 | 1.08 | 0.00 | 0.74 | 15.70 | 25.00 | -43.92 | 74.28 | 0.6960 | -369.0 | -238.8 | |
| 0.00 | 0.90 | 0.00 | 0.62 | 15.93 | 24.72 | -44.20 | 74.01 | 0.6997 | -326.0 | -190.8 | |
| 0.00 | 1.17 | 0.00 | 0.81 | 16.10 | 24.53 | -44.38 | 73.79 | 0.7021 | -425.0 | -352.1 | |
| 0.00 | 0.63 | 0.00 | 0.44 | 17.07 | 23.80 | -45.11 | 72.55 | 0.7123 | -257.0 | -244.7 | |
| 0.00 | 1.17 | 0.00 | 0.82 | 15.44 | 24.05 | -44.86 | 74.80 | 0.7069 | 644.0 | 510.0 | |
| 0.00 | 0.99 | 0.00 | 0.72 | 17.08 | 22.01 | -46.91 | 72.84 | 0.7329 | 528.0 | 506.9 | |
| 0.00 | 0.99 | 0.00 | 0.72 | 15.57 | 21.87 | -47.04 | 74.91 | 0.7325 | 655.0 | 534.9 | |
| 1.62 | 16.32 | 1.19 | 12.02 | 15.61 | 21.21 | -47.71 | 74.94 | 0.7401 | 963.8 | 733.7 | |
| 0.00 | 1.08 | 0.00 | 0.79 | 15.30 | 21.25 | -47.66 | 75.35 | 0.7392 | 417.0 | 361.8 | |
| 6.40 | -24.00 | 4.72 | -24.00 | 15.62 | 20.92 | -47.99 | 74.96 | 0.7433 | 863.1 | 999999 | |
| 0.00 | 1.35 | 0.00 | 1.00 | 16.06 | 20.64 | -48.28 | 74.40 | 0.7469 | 545.0 | 546.3 | |
| 1.71 | 3.97 | 1.28 | 2.97 | 16.16 | 20.27 | -48.64 | 74.32 | 0.7511 | 826.8 | 691.2 | |
| 0.00 | 1.44 | 0.00 | 1.08 | 16.39 | 20.15 | -48.77 | 74.02 | 0.7528 | 704.0 | 638.6 | |
| 0.54 | 2.61 | 0.41 | 1.97 | 16.18 | 19.83 | -49.08 | 74.34 | 0.7560 | 733.2 | 583.1 | |
| 20.73 | 57.52 | 15.60 | 43.25 | 15.53 | 19.90 | -49.02 | 75.19 | 0.7546 | 870.7 | 232.6 | |
| 5.95 | 45.26 | 4.51 | 34.54 | 16.62 | 19.53 | -49.38 | 73.80 | 0.7597 | 798.0 | 238.7 | |
| 4.69 | -32.00 | 3.56 | -32.00 | 16.39 | 19.42 | -49.50 | 74.11 | 0.7607 | 857.4 | 999999 | |
| 2.07 | -32.00 | 1.59 | -32.00 | 16.71 | 19.06 | -49.85 | 73.74 | 0.7649 | 351.1 | 999999 | |
| 0.99 | -32.00 | 0.76 | -32.00 | 16.37 | 19.13 | -49.78 | 74.17 | 0.7638 | 407.7 | 999999 | |
| 0.00 | 1.71 | 0.00 | 1.32 | 16.02 | 18.71 | -50.21 | 74.68 | 0.7680 | -202.0 | -142.3 | |
| 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. | |