| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.54 | 300.26 | 30.74 | 163.44 | 14.78 | 248.77 | -16.95 | 42.77 | 0.4166 | -534.1 | -308.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.01 | 277.76 | 13.07 | 151.00 | 15.06 | 249.05 | -16.67 | 41.88 | 0.4166 | -1115.5 | -402.9 | |
| 29.66 | -1.00 | 16.11 | -1.00 | 14.61 | 249.05 | -16.67 | 42.63 | 0.4115 | -1229.1 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 18.02 | 248.58 | -17.13 | 38.08 | 0.4561 | 775.0 | 639.4 | |
| 2.87 | -1.00 | 1.56 | -1.00 | 14.94 | 248.63 | -17.09 | 42.78 | 0.4197 | -867.1 | 999999 | |
| 0.00 | 2.96 | 0.00 | 1.59 | 12.48 | 248.32 | -17.39 | 47.70 | 0.3962 | 936.0 | 685.6 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 12.97 | 247.24 | -18.47 | 48.46 | 0.4142 | 670.0 | 481.0 | |
| 0.00 | 1.43 | 0.00 | 0.78 | 13.54 | 246.97 | -18.75 | 47.82 | 0.4233 | 660.0 | 519.9 | |
| 0.00 | 2.15 | 0.00 | 1.17 | 13.17 | 246.93 | -18.78 | 48.57 | 0.4199 | 733.0 | 591.3 | |
| 0.00 | 1.79 | 0.00 | 0.98 | 14.09 | 246.76 | -18.95 | 47.17 | 0.4314 | 1009.0 | 855.8 | |
| 0.00 | 1.79 | 0.00 | 0.99 | 15.07 | 246.51 | -19.21 | 45.85 | 0.4446 | 891.0 | 669.6 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 14.22 | 246.35 | -19.36 | 47.53 | 0.4375 | 753.0 | 585.7 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 14.51 | 245.93 | -19.79 | 47.63 | 0.4454 | 784.0 | 732.2 | |
| 0.00 | 1.79 | 0.00 | 0.99 | 14.80 | 245.83 | -19.88 | 47.27 | 0.4494 | 644.0 | 449.6 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 15.26 | 245.39 | -20.33 | 47.13 | 0.4591 | 657.0 | 510.2 | |
| 0.00 | 1.08 | 0.00 | 0.59 | 11.55 | 244.32 | -21.39 | 55.16 | 0.4373 | 613.0 | 426.6 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 16.67 | 240.95 | -24.76 | 50.32 | 0.5234 | 650.0 | 510.1 | |
| 0.00 | 1.43 | 0.00 | 0.83 | 16.58 | 240.76 | -24.96 | 50.67 | 0.5248 | 757.0 | 646.5 | |
| 0.00 | 1.88 | 0.00 | 1.09 | 15.65 | 240.74 | -24.97 | 52.14 | 0.5169 | 774.0 | 650.8 | |
| 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. | |