| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.60 | 0.00 | 17.43 | 13.30 | 58.98 | -62.53 | 78.35 | 0.8834 | 56.6 | 138.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.05 | 0.00 | 1.00 | 14.04 | 62.54 | -58.97 | 77.49 | 0.8536 | -392.0 | -388.2 | |
| 0.00 | 0.97 | 0.00 | 0.99 | 13.44 | 59.78 | -61.73 | 78.21 | 0.8771 | -379.0 | -298.7 | |
| 0.00 | 0.44 | 0.00 | 0.45 | 13.11 | 59.86 | -61.65 | 78.59 | 0.8764 | -483.0 | -382.4 | |
| 0.00 | 0.97 | 0.00 | 1.00 | 13.84 | 59.53 | -61.98 | 77.75 | 0.8791 | -339.0 | -338.8 | |
| 0.00 | 1.58 | 0.00 | 1.64 | 13.55 | 59.40 | -62.11 | 78.08 | 0.8802 | -222.0 | -192.3 | |
| 0.00 | 0.53 | 0.00 | 0.54 | 12.88 | 59.70 | -61.81 | 78.85 | 0.8778 | -119.0 | -169.3 | |
| 0.00 | 1.32 | 0.00 | 1.37 | 13.87 | 59.18 | -62.33 | 77.72 | 0.8819 | -80.0 | -104.9 | |
| 0.00 | 4.04 | 0.00 | 4.23 | 13.40 | 59.07 | -62.44 | 78.25 | 0.8828 | 447.0 | 349.4 | |
| 0.00 | 0.61 | 0.00 | 0.66 | 14.24 | 58.25 | -63.26 | 77.30 | 0.8892 | -234.0 | -259.0 | |
| 0.00 | 2.02 | 0.00 | 2.18 | 12.78 | 58.12 | -63.39 | 78.94 | 0.8903 | 609.0 | 554.2 | |
| 0.00 | 0.26 | 0.00 | 0.28 | 12.57 | 58.14 | -63.37 | 79.18 | 0.8902 | 583.0 | 549.7 | |
| 0.00 | 1.67 | 0.00 | 1.82 | 12.32 | 57.84 | -63.67 | 79.45 | 0.8926 | 600.0 | 531.9 | |
| 0.00 | 0.88 | 0.00 | 0.98 | 13.29 | 57.10 | -64.41 | 78.35 | 0.8981 | 346.0 | 382.5 | |
| 0.00 | 0.26 | 0.00 | 0.29 | 12.70 | 57.31 | -64.20 | 79.02 | 0.8965 | 456.0 | 493.0 | |
| 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. | |