| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.59 | 390.85 | 34.52 | 222.55 | 17.81 | 166.56 | 19.08 | 320.82 | 0.4947 | -819.3 | -314.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.26 | 363.48 | 33.78 | 207.23 | 17.76 | 166.86 | 19.38 | 320.29 | 0.4968 | -1365.9 | -391.4 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 17.26 | 165.30 | 17.83 | 321.93 | 0.4761 | -745.0 | -633.8 | |
| 0.00 | 0.71 | 0.00 | 0.40 | 17.93 | 163.19 | 15.71 | 326.20 | 0.4651 | 682.0 | 526.0 | |
| 0.00 | 1.24 | 0.00 | 0.70 | 18.19 | 163.18 | 15.70 | 326.54 | 0.4683 | 721.0 | 532.5 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 18.28 | 162.92 | 15.45 | 327.08 | 0.4673 | 789.0 | 646.9 | |
| 0.00 | 0.71 | 0.00 | 0.40 | 19.17 | 162.98 | 15.50 | 328.06 | 0.4791 | 705.0 | 532.5 | |
| 1.33 | 6.22 | 0.74 | 3.47 | 17.95 | 162.83 | 15.35 | 326.83 | 0.4623 | 1055.4 | 830.0 | |
| 0.00 | 1.24 | 0.00 | 0.70 | 18.93 | 162.59 | 15.11 | 328.42 | 0.4729 | 700.0 | 610.4 | |
| 0.00 | 1.60 | 0.00 | 0.90 | 19.86 | 162.61 | 15.14 | 329.44 | 0.4850 | 633.0 | 552.0 | |
| 0.00 | 1.87 | 0.00 | 1.04 | 18.53 | 162.42 | 14.95 | 328.23 | 0.4664 | 772.0 | 595.0 | |
| 0.00 | 1.07 | 0.00 | 0.60 | 18.73 | 162.37 | 14.90 | 328.55 | 0.4685 | 616.0 | 492.7 | |
| 0.00 | 3.20 | 0.00 | 1.81 | 19.98 | 162.39 | 14.92 | 329.94 | 0.4850 | 731.0 | 582.8 | |
| 0.00 | 6.22 | 0.00 | 3.47 | 18.36 | 161.98 | 14.50 | 328.79 | 0.4606 | 789.0 | 621.6 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 17.12 | 160.44 | 12.97 | 330.09 | 0.4319 | 849.0 | 773.5 | |
| 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. | |