SDO HMI 2014-08-14 15:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.96 | 327.10 | 38.34 | 221.39 | 14.85 | 133.33 | 42.93 | 284.65 | 0.6824 | -613.7 | -237.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.79 | 291.33 | 31.40 | 199.61 | 15.36 | 134.15 | 43.75 | 285.35 | 0.6938 | -1156.8 | -318.4 | |
| 2.61 | -1.00 | 1.77 | -1.00 | 14.94 | 133.57 | 43.16 | 284.84 | 0.6860 | -1032.8 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.67 | 16.18 | 133.50 | 43.10 | 286.66 | 0.6872 | -283.0 | -254.9 | |
| 0.00 | 0.99 | 0.00 | 0.65 | 13.31 | 131.45 | 41.05 | 282.73 | 0.6574 | -561.0 | -457.7 | |
| 0.00 | 1.53 | 0.00 | 0.96 | 12.81 | 128.08 | 37.68 | 282.46 | 0.6126 | 748.0 | 650.3 | |
| 0.00 | 1.53 | 0.00 | 0.93 | 9.60 | 126.32 | 35.91 | 277.28 | 0.5852 | 557.0 | 467.8 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 9.67 | 126.18 | 35.77 | 277.41 | 0.5833 | 795.0 | 633.8 | |
| 1.44 | 23.89 | 0.87 | 14.44 | 9.97 | 125.83 | 35.43 | 277.95 | 0.5786 | 687.6 | 664.7 | |
| 6.67 | -8.00 | 4.03 | -8.00 | 9.99 | 125.50 | 35.09 | 278.01 | 0.5739 | 1007.5 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.14 | 9.56 | 125.44 | 35.04 | 277.28 | 0.5729 | 890.0 | 731.6 | |
| 0.00 | 1.17 | 0.00 | 0.71 | 10.78 | 125.60 | 35.19 | 279.38 | 0.5760 | 679.0 | 536.1 | |
| 0.45 | 2.43 | 0.27 | 1.47 | 9.20 | 125.36 | 34.96 | 276.65 | 0.5716 | 852.4 | 697.2 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 11.14 | 122.34 | 31.93 | 280.50 | 0.5298 | 531.0 | 543.3 | |
| 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. | |