SDO HMI 2014-12-07 08:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.73 | 550.83 | 133.26 | 798.74 | -19.60 | 85.54 | 68.66 | 249.03 | 0.9410 | 573.6 | 207.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.33 | 543.31 | 44.50 | 789.19 | -18.78 | 87.33 | 70.45 | 250.13 | 0.9501 | 393.4 | 207.1 | |
| 20.48 | -1.00 | 29.73 | -1.00 | -19.18 | 85.70 | 68.83 | 249.51 | 0.9417 | 670.5 | 999999 | |
| 2.30 | -1.00 | 3.25 | -1.00 | -19.55 | 84.83 | 67.95 | 249.00 | 0.9371 | 571.9 | 999999 | |
| 1.28 | -1.00 | 1.89 | -1.00 | -20.82 | 85.85 | 68.97 | 247.80 | 0.9437 | -186.9 | 999999 | |
| 1.54 | -1.00 | 2.14 | -1.00 | -19.74 | 84.66 | 67.78 | 248.78 | 0.9363 | 477.7 | 999999 | |
| 0.00 | 0.85 | 0.00 | 1.09 | -17.80 | 82.71 | 65.83 | 250.58 | 0.9228 | -249.0 | -238.4 | |
| 0.00 | 1.11 | 0.00 | 1.42 | -18.64 | 82.79 | 65.91 | 249.69 | 0.9241 | 366.0 | 319.7 | |
| 36.60 | -1.00 | 50.07 | -1.00 | -20.40 | 84.08 | 67.21 | 248.00 | 0.9335 | 784.0 | 999999 | |
| 0.94 | -1.00 | 1.33 | -1.00 | -21.77 | 84.78 | 67.90 | 246.65 | 0.9388 | 433.1 | 999999 | |
| 0.26 | -1.00 | 0.35 | -1.00 | -21.67 | 84.10 | 67.22 | 246.65 | 0.9348 | 110.3 | 999999 | |
| 0.00 | 4.27 | 0.00 | 5.50 | -21.95 | 82.35 | 65.47 | 246.07 | 0.9248 | 547.0 | 361.7 | |
| 0.00 | 0.26 | 0.00 | 0.32 | -20.96 | 81.51 | 64.63 | 246.99 | 0.9184 | 350.0 | 284.7 | |
| 0.00 | 0.26 | 0.00 | 0.30 | -19.57 | 80.30 | 63.42 | 248.28 | 0.9088 | -298.0 | -228.3 | |
| 0.00 | 0.77 | 0.00 | 0.92 | -21.15 | 80.63 | 63.75 | 246.63 | 0.9130 | -210.0 | -129.2 | |
| 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. | |