| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43 | 482 | 33 | 368 | 9.72 | 267.97 | -49.88 | 81.01 | 0.7652 | 866.3 | 295.5 | |
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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 | 10.35 | 271.97 | -45.88 | 79.87 | 0.7197 | 668.0 | 626.4 | |
| 0 | 4 | 0 | 3 | 8.49 | 271.50 | -46.35 | 82.47 | 0.7242 | 453.0 | 459.7 | |
| 0 | 20 | 0 | 14 | 9.88 | 270.52 | -47.33 | 80.63 | 0.7365 | 639.0 | 586.4 | |
| 0 | 3 | 0 | 2 | 9.31 | 270.10 | -47.75 | 81.43 | 0.7411 | 514.0 | 521.0 | |
| 3 | 15 | 2 | 11 | 8.96 | 269.40 | -48.45 | 81.94 | 0.7490 | 471.3 | 521.2 | |
| 0 | 5 | 0 | 4 | 6.38 | 269.67 | -48.17 | 85.40 | 0.7453 | 363.0 | 285.7 | |
| 20 | 395 | 15 | 302 | 9.77 | 268.59 | -49.26 | 80.91 | 0.7585 | 1452.9 | 337.8 | |
| 3 | -7 | 2 | -7 | 9.58 | 268.02 | -49.83 | 81.19 | 0.7648 | 776.2 | 999999 | |
| 7 | -7 | 6 | -7 | 9.96 | 267.88 | -49.97 | 80.69 | 0.7665 | 979.3 | 999999 | |
| 3 | -7 | 3 | -7 | 9.71 | 267.57 | -50.28 | 81.04 | 0.7699 | 640.7 | 999999 | |
| 7 | -7 | 5 | -7 | 9.04 | 266.90 | -50.95 | 81.93 | 0.7770 | -339.6 | 999999 | |
| 0 | 5 | 0 | 4 | 7.12 | 266.55 | -51.30 | 84.41 | 0.7804 | -663.0 | -520.7 | |
| 0 | 8 | 0 | 7 | 12.36 | 264.21 | -53.64 | 77.90 | 0.8068 | -594.0 | -379.7 | |
| 0 | 9 | 0 | 7 | 10.79 | 264.25 | -53.60 | 79.83 | 0.8055 | -499.0 | -393.8 | |
| 0 | 6 | 0 | 5 | 11.39 | 263.82 | -54.03 | 79.12 | 0.8102 | -567.0 | -437.7 | |
| 0 | 8 | 0 | 6 | 11.71 | 263.32 | -54.53 | 78.75 | 0.8153 | -656.0 | -494.2 | |
| 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. | |