| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.31 | 44.02 | 9.68 | 31.73 | -19.48 | 258.32 | 38.78 | 234.33 | 0.7287 | 284.0 | 259.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.25 | 0.00 | 0.95 | -20.70 | 260.66 | 41.12 | 234.45 | 0.7584 | 591.0 | 518.3 | |
| 0.00 | 0.89 | 0.00 | 0.66 | -20.07 | 259.19 | 39.65 | 234.23 | 0.7409 | 365.0 | 283.9 | |
| 10.36 | 26.08 | 7.54 | 18.96 | -19.48 | 258.97 | 39.43 | 234.78 | 0.7352 | 774.3 | 638.4 | |
| 0.00 | 1.34 | 0.00 | 0.98 | -20.05 | 259.01 | 39.47 | 234.14 | 0.7392 | 641.0 | 522.1 | |
| 2.95 | -3.00 | 2.14 | -3.00 | -19.72 | 258.67 | 39.12 | 234.29 | 0.7338 | 755.5 | 999999 | |
| 0.00 | 1.96 | 0.00 | 1.46 | -21.61 | 258.96 | 39.42 | 232.32 | 0.7483 | 503.0 | 373.6 | |
| 0.00 | 2.68 | 0.00 | 1.94 | -19.76 | 258.35 | 38.81 | 234.03 | 0.7310 | 602.0 | 478.3 | |
| 0.00 | 2.86 | 0.00 | 2.02 | -18.88 | 257.49 | 37.95 | 234.48 | 0.7171 | -475.0 | -281.3 | |
| 0.00 | 1.16 | 0.00 | 0.81 | -18.57 | 256.88 | 37.34 | 234.44 | 0.7091 | -648.0 | -561.2 | |
| 0.00 | 1.07 | 0.00 | 0.74 | -19.32 | 255.79 | 36.25 | 232.76 | 0.7033 | -454.0 | -384.3 | |
| 0.00 | 0.89 | 0.00 | 0.62 | -19.55 | 255.77 | 36.23 | 232.46 | 0.7047 | -575.0 | -538.7 | |
| 0.00 | 1.34 | 0.00 | 0.91 | -17.86 | 255.08 | 35.54 | 233.99 | 0.6862 | -612.0 | -470.1 | |
| 0.00 | 1.07 | 0.00 | 0.72 | -17.64 | 254.75 | 35.21 | 234.03 | 0.6813 | -688.0 | -514.6 | |
| 0.00 | 1.43 | 0.00 | 0.96 | -17.41 | 254.35 | 34.81 | 234.01 | 0.6756 | -548.0 | -429.9 | |
| 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. | |