| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.60 | 57.60 | 16.74 | 48.00 | 7.86 | 134.66 | 51.48 | 285.45 | 0.8056 | 128.7 | 338.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.50 | 14.51 | 8.65 | 13.22 | 7.33 | 138.49 | 55.31 | 283.63 | 0.8413 | -636.4 | -296.8 | |
| 0.00 | 2.50 | 0.00 | 2.13 | 8.30 | 135.40 | 52.23 | 285.68 | 0.8146 | 505.0 | 302.8 | |
| 0.00 | 0.86 | 0.00 | 0.71 | 6.24 | 134.72 | 51.54 | 283.42 | 0.8026 | -647.0 | -519.7 | |
| 0.00 | 1.21 | 0.00 | 1.01 | 7.72 | 134.86 | 51.68 | 285.17 | 0.8078 | 385.0 | 347.5 | |
| 0.00 | 1.90 | 0.00 | 1.57 | 7.43 | 134.42 | 51.24 | 284.96 | 0.8026 | 586.0 | 530.9 | |
| 0.00 | 1.55 | 0.00 | 1.28 | 7.23 | 134.19 | 51.02 | 284.78 | 0.7998 | 467.0 | 430.2 | |
| 0.00 | 1.30 | 0.00 | 1.05 | 6.64 | 133.87 | 50.69 | 284.17 | 0.7950 | -231.0 | -354.4 | |
| 0.00 | 0.95 | 0.00 | 0.78 | 8.87 | 133.82 | 50.64 | 286.89 | 0.8007 | 412.0 | 333.8 | |
| 0.00 | 2.07 | 0.00 | 1.69 | 8.78 | 133.51 | 50.34 | 286.89 | 0.7974 | 581.0 | 507.3 | |
| 0.00 | 0.95 | 0.00 | 0.77 | 8.32 | 133.15 | 49.97 | 286.45 | 0.7923 | 341.0 | 271.5 | |
| 0.43 | 2.25 | 0.35 | 1.80 | 7.81 | 133.01 | 49.84 | 285.88 | 0.7894 | 479.2 | 318.3 | |
| 4.75 | 27.55 | 3.80 | 21.99 | 8.09 | 132.73 | 49.56 | 286.32 | 0.7874 | 704.7 | 597.3 | |
| 2.59 | -12.00 | 2.08 | -12.00 | 8.43 | 132.74 | 49.57 | 286.73 | 0.7885 | 825.2 | 999999 | |
| 2.33 | -12.00 | 1.86 | -12.00 | 8.22 | 132.43 | 49.25 | 286.58 | 0.7846 | 809.9 | 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. | |