| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93 | 578 | 72 | 471 | 13.20 | 359.00 | 53.13 | 281.12 | 0.7949 | 362.8 | 248.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 3 | 12.10 | 2.78 | 56.91 | 279.74 | 0.8333 | -128.0 | -151.5 | |
| 12 | 164 | 11 | 144 | 13.18 | 2.41 | 56.54 | 281.03 | 0.8298 | 585.0 | 289.7 | |
| 6 | -2 | 5 | -2 | 13.03 | 1.92 | 56.05 | 280.85 | 0.8251 | 871.1 | 999999 | |
| 6 | -2 | 5 | -2 | 13.93 | 2.10 | 56.23 | 281.95 | 0.8269 | 541.9 | 999999 | |
| 0 | 7 | 0 | 6 | 12.32 | 0.34 | 54.47 | 279.98 | 0.8095 | 566.0 | 485.2 | |
| 2 | 14 | 1 | 12 | 11.81 | 359.84 | 53.97 | 279.34 | 0.8045 | 681.0 | 587.9 | |
| 0 | 4 | 0 | 3 | 12.60 | 359.94 | 54.07 | 280.32 | 0.8055 | 284.0 | 363.2 | |
| 14 | 169 | 11 | 138 | 13.80 | 359.44 | 53.57 | 281.84 | 0.8006 | 1025.1 | 580.8 | |
| 7 | -8 | 5 | -8 | 13.69 | 358.92 | 53.06 | 281.72 | 0.7953 | 1439.1 | 999999 | |
| 8 | 63 | 6 | 50 | 11.71 | 358.07 | 52.20 | 279.21 | 0.7861 | -548.1 | -56.6 | |
| 13 | 61 | 10 | 48 | 12.78 | 357.71 | 51.85 | 280.58 | 0.7824 | -615.7 | 166.2 | |
| 9 | -11 | 7 | -11 | 13.33 | 357.35 | 51.49 | 281.30 | 0.7787 | 780.2 | 999999 | |
| 7 | 15 | 5 | 12 | 13.52 | 356.25 | 50.38 | 281.58 | 0.7669 | 634.8 | 434.0 | |
| 4 | 42 | 3 | 30 | 13.65 | 352.26 | 46.39 | 281.99 | 0.7217 | -769.1 | -209.3 | |
| 0 | 3 | 0 | 2 | 12.75 | 352.04 | 46.17 | 280.75 | 0.7185 | -511.0 | -432.9 | |
| 5 | 32 | 3 | 23 | 13.15 | 351.61 | 45.74 | 281.33 | 0.7137 | -1055.7 | -818.9 | |
| 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. | |