| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.33 | 202.93 | 18.99 | 103.13 | 13.62 | 291.61 | 11.51 | 300.67 | 0.2268 | -765.4 | -436.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.46 | 13.76 | 292.80 | 12.71 | 298.81 | 0.2449 | -772.0 | -537.6 | |
| 0.00 | 1.25 | 0.00 | 0.64 | 13.56 | 292.38 | 12.28 | 298.82 | 0.2371 | -736.0 | -572.0 | |
| 8.32 | 191.74 | 4.23 | 97.46 | 13.23 | 291.92 | 11.82 | 298.44 | 0.2277 | -1127.2 | -480.8 | |
| 1.97 | -3.00 | 1.00 | -3.00 | 12.96 | 291.87 | 11.77 | 297.43 | 0.2250 | -966.9 | 999999 | |
| 7.70 | -3.00 | 3.92 | -3.00 | 14.06 | 291.86 | 11.76 | 301.72 | 0.2336 | -1075.6 | 999999 | |
| 11.91 | -3.00 | 6.06 | -3.00 | 13.60 | 291.71 | 11.61 | 300.29 | 0.2276 | -1127.7 | 999999 | |
| 5.82 | -3.00 | 2.96 | -3.00 | 13.30 | 291.60 | 11.50 | 299.33 | 0.2236 | -1379.3 | 999999 | |
| 1.61 | -3.00 | 0.82 | -3.00 | 13.34 | 291.38 | 11.28 | 299.92 | 0.2207 | -1263.4 | 999999 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 13.80 | 291.06 | 10.96 | 302.47 | 0.2198 | -838.0 | -703.5 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 11.90 | 290.19 | 10.09 | 296.17 | 0.1918 | 866.0 | 605.1 | |
| 0.00 | 1.79 | 0.00 | 0.90 | 15.57 | 287.80 | 7.70 | 318.71 | 0.1966 | 829.0 | 673.2 | |
| 0.00 | 2.51 | 0.00 | 1.27 | 16.60 | 287.05 | 6.95 | 324.81 | 0.2021 | 270.0 | 343.5 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 16.57 | 286.76 | 6.66 | 325.85 | 0.1990 | 927.0 | 719.1 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 17.37 | 286.57 | 6.47 | 328.82 | 0.2086 | 699.0 | 586.4 | |
| 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. | |