| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.98 | 0.00 | 13.09 | 16.81 | 326.44 | 0.68 | 357.48 | 0.1808 | 432.3 | 349.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.88 | 0.00 | 0.95 | 15.79 | 332.93 | 7.17 | 321.56 | 0.1942 | -995.0 | -779.2 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 17.61 | 332.33 | 6.57 | 329.15 | 0.2137 | -996.0 | -780.2 | |
| 0.00 | 1.25 | 0.00 | 0.64 | 19.53 | 329.38 | 3.61 | 344.54 | 0.2239 | -960.0 | -809.4 | |
| 0.00 | 2.42 | 0.00 | 1.22 | 17.40 | 328.66 | 2.90 | 344.84 | 0.1856 | 822.0 | 750.0 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 17.34 | 328.50 | 2.74 | 345.55 | 0.1839 | 1112.0 | 936.9 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 17.68 | 328.19 | 2.43 | 347.56 | 0.1884 | 1020.0 | 724.1 | |
| 0.00 | 2.33 | 0.00 | 1.18 | 19.20 | 327.28 | 1.52 | 353.16 | 0.2115 | -858.0 | -617.2 | |
| 0.00 | 4.48 | 0.00 | 2.25 | 16.34 | 326.79 | 1.02 | 353.87 | 0.1615 | 1049.0 | 832.5 | |
| 0.00 | 1.97 | 0.00 | 0.99 | 15.94 | 326.25 | 0.49 | 356.94 | 0.1539 | 1033.0 | 848.5 | |
| 0.00 | 1.88 | 0.00 | 0.94 | 13.46 | 323.66 | -2.10 | 17.93 | 0.1164 | 869.0 | 662.9 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 13.09 | 322.01 | -3.75 | 31.50 | 0.1224 | 887.0 | 682.5 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 13.24 | 321.85 | -3.91 | 31.90 | 0.1260 | 924.0 | 686.4 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 14.79 | 321.61 | -4.15 | 27.68 | 0.1514 | 731.0 | 633.4 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 18.61 | 319.95 | -5.81 | 25.67 | 0.2223 | 984.0 | 737.7 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 19.50 | 318.99 | -6.78 | 27.37 | 0.2430 | 863.0 | 625.8 | |
| 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. | |