| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.12 | 173.44 | 29.37 | 110.58 | 33.97 | 267.74 | 12.93 | 342.82 | 0.6313 | -31.3 | -79.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.33 | 99.81 | 11.07 | 63.82 | 33.60 | 269.71 | 14.90 | 340.18 | 0.6342 | -1043.5 | -357.7 | |
| 1.78 | -1.00 | 1.13 | -1.00 | 33.37 | 269.15 | 14.35 | 340.71 | 0.6289 | -739.0 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 32.93 | 268.97 | 14.17 | 340.65 | 0.6225 | -736.0 | -646.6 | |
| 1.87 | 3.82 | 1.19 | 2.43 | 33.62 | 268.72 | 13.92 | 341.39 | 0.6301 | -756.7 | -729.8 | |
| 0.00 | 0.93 | 0.00 | 0.60 | 34.03 | 268.75 | 13.95 | 341.60 | 0.6353 | -556.0 | -467.8 | |
| 0.34 | -4.00 | 0.22 | -4.00 | 33.80 | 268.64 | 13.84 | 341.60 | 0.6321 | -807.2 | 999999 | |
| 0.00 | 2.38 | 0.00 | 1.52 | 34.52 | 266.74 | 11.94 | 344.33 | 0.6336 | -744.0 | -641.2 | |
| 0.00 | 0.51 | 0.00 | 0.32 | 33.19 | 266.27 | 11.46 | 344.24 | 0.6146 | 686.0 | 534.0 | |
| 1.78 | 9.85 | 1.12 | 6.17 | 33.43 | 265.00 | 10.20 | 346.00 | 0.6133 | 890.8 | 679.9 | |
| 1.10 | 2.55 | 0.71 | 1.63 | 35.02 | 265.13 | 10.33 | 346.58 | 0.6347 | 539.0 | 467.9 | |
| 2.04 | 11.81 | 1.31 | 7.58 | 35.47 | 264.97 | 10.16 | 346.97 | 0.6400 | 722.1 | 615.1 | |
| 4.08 | 39.92 | 2.58 | 25.34 | 34.27 | 264.67 | 9.87 | 346.82 | 0.6234 | 949.6 | 500.8 | |
| 0.00 | 0.59 | 0.00 | 0.37 | 33.98 | 264.64 | 9.83 | 346.73 | 0.6194 | 656.0 | 614.7 | |
| 15.80 | -12.00 | 10.04 | -12.00 | 34.68 | 264.50 | 9.70 | 347.21 | 0.6283 | 904.5 | 999999 | |
| 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. | |