| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.70 | 320.98 | 44.33 | 238.89 | 12.43 | 13.73 | -44.71 | 66.97 | 0.7487 | -771.7 | -286.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.44 | 0.00 | 0.30 | 4.17 | 15.59 | -42.84 | 77.16 | 0.6979 | 551.0 | 470.0 | |
| 53.38 | 305.61 | 39.54 | 226.87 | 12.46 | 14.02 | -44.42 | 66.80 | 0.7458 | -1147.3 | -331.5 | |
| 0.00 | 0.97 | 0.00 | 0.67 | 2.75 | 15.13 | -43.30 | 79.30 | 0.6995 | 456.0 | 460.5 | |
| 0.53 | -2.00 | 0.40 | -2.00 | 12.80 | 12.98 | -45.45 | 66.85 | 0.7581 | -340.7 | 999999 | |
| 0.00 | 1.67 | 0.00 | 1.27 | 13.51 | 12.77 | -45.67 | 66.07 | 0.7632 | 223.0 | 114.1 | |
| 5.79 | -2.00 | 4.39 | -2.00 | 12.62 | 12.85 | -45.59 | 67.14 | 0.7588 | -512.0 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.94 | 13.39 | 12.66 | -45.77 | 66.26 | 0.7638 | 170.0 | 122.6 | |
| 0.00 | 0.53 | 0.00 | 0.40 | 11.91 | 12.34 | -46.09 | 68.24 | 0.7613 | -265.0 | -220.8 | |
| 0.00 | 1.05 | 0.00 | 0.81 | 11.00 | 11.29 | -47.15 | 69.81 | 0.7691 | 588.0 | 490.2 | |
| 0.00 | 2.90 | 0.00 | 2.25 | 11.03 | 10.92 | -47.52 | 69.91 | 0.7730 | 614.0 | 541.0 | |
| 0.00 | 1.05 | 0.00 | 0.83 | 11.64 | 10.74 | -47.70 | 69.24 | 0.7770 | 681.0 | 609.9 | |
| 0.00 | 1.76 | 0.00 | 1.38 | 11.32 | 10.49 | -47.95 | 69.73 | 0.7784 | 495.0 | 355.0 | |
| 0.00 | 2.28 | 0.00 | 1.92 | 12.93 | 7.87 | -50.57 | 68.80 | 0.8097 | 573.0 | 516.1 | |
| 0.00 | 1.49 | 0.00 | 1.25 | 12.78 | 7.76 | -50.67 | 69.01 | 0.8102 | 532.0 | 436.7 | |
| 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. | |