| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.41 | 44.99 | 10.21 | 33.86 | 15.57 | 54.00 | 48.98 | 284.79 | 0.7528 | 54.8 | -142.9 | |
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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 | 0.78 | 9.51 | 60.53 | 55.50 | 276.80 | 0.8207 | -429.0 | -398.9 | |
| 0.00 | 2.70 | 0.00 | 2.21 | 14.19 | 58.37 | 53.35 | 282.59 | 0.7992 | -674.0 | -596.8 | |
| 4.50 | 7.02 | 3.70 | 5.78 | 14.68 | 58.49 | 53.47 | 283.20 | 0.8006 | -671.3 | -458.5 | |
| 0.00 | 1.08 | 0.00 | 0.87 | 16.88 | 57.22 | 52.20 | 286.07 | 0.7891 | -376.0 | -335.8 | |
| 0.00 | 0.54 | 0.00 | 0.41 | 14.12 | 54.86 | 49.83 | 282.69 | 0.7619 | 371.0 | 362.5 | |
| 0.00 | 0.81 | 0.00 | 0.62 | 14.25 | 54.75 | 49.72 | 282.87 | 0.7608 | 493.0 | 395.4 | |
| 2.07 | 13.31 | 1.57 | 10.05 | 15.95 | 54.42 | 49.39 | 285.15 | 0.7585 | -555.8 | -591.4 | |
| 1.53 | -7.00 | 1.15 | -7.00 | 15.83 | 54.13 | 49.11 | 285.01 | 0.7553 | -845.8 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.65 | 15.76 | 52.03 | 47.00 | 285.16 | 0.7316 | -224.0 | -169.7 | |
| 4.86 | 7.20 | 3.48 | 5.16 | 15.90 | 51.47 | 46.44 | 285.43 | 0.7253 | 576.0 | 302.0 | |
| 0.00 | 0.54 | 0.00 | 0.38 | 14.61 | 51.05 | 46.03 | 283.68 | 0.7190 | 414.0 | 491.7 | |
| 0.00 | 1.80 | 0.00 | 1.26 | 16.18 | 50.05 | 45.03 | 286.01 | 0.7092 | 660.0 | 572.0 | |
| 0.00 | 1.26 | 0.00 | 0.89 | 16.98 | 50.16 | 45.13 | 287.12 | 0.7116 | 278.0 | 278.0 | |
| 0.00 | 1.08 | 0.00 | 0.76 | 17.44 | 50.30 | 45.28 | 287.73 | 0.7140 | 514.0 | 391.0 | |
| 0.45 | 2.79 | 0.31 | 1.94 | 16.30 | 49.69 | 44.66 | 286.25 | 0.7050 | 771.2 | 420.0 | |
| 0.00 | 1.08 | 0.00 | 0.73 | 13.67 | 47.79 | 42.76 | 282.72 | 0.6786 | 598.0 | 466.4 | |
| 0.00 | 1.08 | 0.00 | 0.75 | 18.40 | 48.86 | 43.84 | 289.37 | 0.6989 | 497.0 | 387.8 | |
| 0.00 | 0.90 | 0.00 | 0.62 | 20.05 | 47.90 | 42.88 | 291.95 | 0.6914 | 520.0 | 458.3 | |
| 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. | |