| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.14 | 35.24 | 6.81 | 19.79 | -15.56 | 246.37 | -22.96 | 126.96 | 0.4699 | 103.6 | 227.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.36 | 3.08 | 0.74 | 1.68 | -15.40 | 250.34 | -18.99 | 131.37 | 0.4198 | 970.2 | 751.3 | |
| 3.62 | 11.50 | 1.98 | 6.28 | -15.27 | 250.12 | -19.21 | 130.82 | 0.4212 | 972.6 | 725.8 | |
| 2.45 | -2.00 | 1.33 | -2.00 | -15.08 | 249.97 | -19.36 | 130.25 | 0.4212 | 950.0 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -15.18 | 249.49 | -19.84 | 129.77 | 0.4279 | 705.0 | 472.2 | |
| 0.00 | 1.99 | 0.00 | 1.11 | -15.03 | 247.17 | -22.16 | 126.55 | 0.4552 | 890.0 | 672.6 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -15.38 | 246.86 | -22.47 | 126.82 | 0.4622 | 716.0 | 622.6 | |
| 0.00 | 2.54 | 0.00 | 1.43 | -14.82 | 245.17 | -24.16 | 123.95 | 0.4788 | 796.0 | 570.4 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -15.27 | 244.77 | -24.56 | 124.32 | 0.4874 | 639.0 | 491.9 | |
| 0.00 | 2.08 | 0.00 | 1.20 | -15.59 | 243.33 | -26.00 | 123.46 | 0.5081 | -813.0 | -679.2 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -15.98 | 242.75 | -26.58 | 123.57 | 0.5183 | -821.0 | -566.6 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -15.69 | 242.40 | -26.93 | 122.77 | 0.5206 | -797.0 | -628.4 | |
| 0.00 | 0.82 | 0.00 | 0.47 | -16.01 | 242.10 | -27.23 | 123.04 | 0.5266 | -869.0 | -744.6 | |
| 4.71 | 5.07 | 2.76 | 2.97 | -16.68 | 241.71 | -27.61 | 123.79 | 0.5363 | -815.9 | -633.5 | |
| 0.00 | 1.99 | 0.00 | 1.17 | -16.33 | 241.66 | -27.67 | 123.17 | 0.5344 | -360.0 | -412.5 | |
| 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. | |