| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.40 | 260.14 | 60.46 | 357.89 | 15.56 | 279.08 | -69.33 | 75.39 | 0.9318 | -253.1 | 14.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.86 | 15.25 | 288.37 | -60.04 | 75.51 | 0.8654 | -419.0 | -368.7 | |
| 0.00 | 1.57 | 0.00 | 1.64 | 12.65 | 286.14 | -62.27 | 78.56 | 0.8831 | -444.0 | -338.2 | |
| 10.62 | 189.44 | 13.22 | 243.98 | 15.76 | 281.25 | -67.16 | 75.17 | 0.9192 | -758.8 | -67.2 | |
| 4.27 | -3.00 | 5.46 | -3.00 | 16.14 | 280.58 | -67.83 | 74.77 | 0.9237 | -236.6 | 999999 | |
| 8.62 | -3.00 | 11.02 | -3.00 | 15.43 | 280.58 | -67.84 | 75.54 | 0.9236 | -439.0 | 999999 | |
| 9.49 | -3.00 | 12.24 | -3.00 | 14.83 | 280.40 | -68.01 | 76.19 | 0.9247 | -551.0 | 999999 | |
| 1.22 | 34.48 | 1.70 | 47.99 | 17.11 | 278.59 | -69.82 | 73.75 | 0.9359 | 636.0 | 480.0 | |
| 2.26 | -3.00 | 2.97 | -3.00 | 14.88 | 279.94 | -68.47 | 76.14 | 0.9276 | 149.6 | 999999 | |
| 0.26 | -7.00 | 0.37 | -7.00 | 16.54 | 278.43 | -69.98 | 74.36 | 0.9369 | -51.7 | 999999 | |
| 1.65 | -7.00 | 2.33 | -7.00 | 16.62 | 278.27 | -70.14 | 74.28 | 0.9378 | 359.7 | 999999 | |
| 0.00 | 1.04 | 0.00 | 1.82 | 15.71 | 274.02 | -74.39 | 75.20 | 0.9602 | 307.0 | 298.3 | |
| 0.00 | 1.22 | 0.00 | 2.12 | 15.26 | 274.13 | -74.28 | 75.68 | 0.9597 | 410.0 | 356.3 | |
| 6.01 | 31.52 | 11.15 | 59.48 | 15.25 | 273.05 | -75.36 | 75.66 | 0.9647 | 375.8 | -73.8 | |
| 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. | |