| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.02 | 452.90 | 33.58 | 245.01 | 16.65 | 110.02 | 17.90 | 312.92 | 0.4039 | -916.0 | -332.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.02 | 429.24 | 33.58 | 232.41 | 16.59 | 110.27 | 18.15 | 312.36 | 0.4058 | -1584.7 | -396.5 | |
| 0.00 | 2.56 | 0.00 | 1.38 | 17.90 | 107.55 | 15.43 | 319.26 | 0.3897 | 745.0 | 634.6 | |
| 0.00 | 2.22 | 0.00 | 1.19 | 17.07 | 107.15 | 15.04 | 318.47 | 0.3757 | 750.0 | 561.8 | |
| 0.00 | 0.43 | 0.00 | 0.23 | 18.09 | 107.11 | 15.00 | 320.37 | 0.3874 | 661.0 | 595.4 | |
| 0.00 | 2.31 | 0.00 | 1.23 | 17.47 | 106.84 | 14.72 | 319.80 | 0.3771 | 769.0 | 725.3 | |
| 0.00 | 2.90 | 0.00 | 1.55 | 17.72 | 106.79 | 14.68 | 320.32 | 0.3796 | 1002.0 | 822.5 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 17.94 | 106.62 | 14.50 | 321.03 | 0.3804 | 728.0 | 621.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 17.16 | 106.55 | 14.44 | 319.77 | 0.3705 | 832.0 | 657.0 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 17.11 | 105.31 | 13.19 | 322.14 | 0.3569 | 999.0 | 807.6 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 17.27 | 104.75 | 12.63 | 323.59 | 0.3534 | 967.0 | 882.6 | |
| 0.00 | 3.59 | 0.00 | 1.90 | 17.36 | 104.21 | 12.10 | 324.91 | 0.3495 | 942.0 | 661.0 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 19.35 | 103.34 | 11.22 | 329.98 | 0.3686 | 610.0 | 502.8 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 19.41 | 102.00 | 9.89 | 333.07 | 0.3592 | 742.0 | 603.3 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 19.38 | 101.78 | 9.66 | 333.56 | 0.3571 | 802.0 | 629.3 | |
| 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. | |