| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.39 | 70.10 | 25.64 | 60.67 | 19.74 | 64.66 | 48.95 | 300.02 | 0.8210 | 192.7 | 233.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.11 | 18.77 | 9.56 | 17.82 | 19.01 | 68.92 | 53.21 | 297.30 | 0.8541 | -639.8 | 18.7 | |
| 0.00 | 1.11 | 0.00 | 1.00 | 18.47 | 67.04 | 51.32 | 297.48 | 0.8367 | -549.0 | -509.0 | |
| 0.00 | 1.54 | 0.00 | 1.39 | 18.83 | 67.09 | 51.37 | 297.86 | 0.8385 | -645.0 | -536.5 | |
| 0.00 | 1.03 | 0.00 | 0.89 | 18.94 | 65.16 | 49.44 | 298.82 | 0.8224 | 402.0 | 357.5 | |
| 0.00 | 1.11 | 0.00 | 0.95 | 19.88 | 63.72 | 48.01 | 300.54 | 0.8138 | 419.0 | 380.0 | |
| 0.00 | 1.11 | 0.00 | 0.95 | 20.07 | 63.66 | 47.94 | 300.79 | 0.8140 | 210.0 | 318.6 | |
| 0.00 | 1.89 | 0.00 | 1.60 | 20.22 | 63.53 | 47.81 | 301.02 | 0.8136 | 401.0 | 336.2 | |
| 3.26 | 3.86 | 2.74 | 3.25 | 19.98 | 63.38 | 47.67 | 300.82 | 0.8113 | 530.7 | 471.6 | |
| 8.40 | 20.91 | 6.97 | 17.34 | 19.88 | 62.69 | 46.98 | 301.05 | 0.8048 | 782.3 | 331.9 | |
| 1.11 | 1.54 | 0.96 | 1.33 | 21.87 | 63.47 | 47.76 | 302.87 | 0.8203 | -499.2 | -346.6 | |
| 6.51 | 12.77 | 5.41 | 10.59 | 20.26 | 62.52 | 46.80 | 301.57 | 0.8049 | 761.4 | 486.8 | |
| 0.00 | 0.86 | 0.00 | 0.70 | 20.98 | 61.01 | 45.30 | 303.16 | 0.7950 | 507.0 | 402.3 | |
| 0.00 | 0.86 | 0.00 | 0.69 | 20.64 | 60.57 | 44.85 | 303.02 | 0.7894 | 343.0 | 412.4 | |
| 0.00 | 1.37 | 0.00 | 1.09 | 20.70 | 60.05 | 44.34 | 303.36 | 0.7851 | 635.0 | 477.5 | |
| 0.00 | 1.37 | 0.00 | 1.08 | 20.76 | 59.68 | 43.96 | 303.64 | 0.7820 | 715.0 | 553.2 | |
| 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. | |