| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.81 | 414.38 | 37.25 | 218.07 | 12.69 | 13.54 | 5.46 | 344.01 | 0.3382 | -1123.2 | -427.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.58 | 0.00 | 0.84 | 14.26 | 15.02 | 6.93 | 341.47 | 0.3697 | 746.0 | 658.1 | |
| 68.26 | 396.62 | 35.90 | 208.72 | 12.65 | 13.64 | 5.56 | 343.69 | 0.3379 | -1559.9 | -454.5 | |
| 2.55 | -2.00 | 1.35 | -2.00 | 13.25 | 13.31 | 5.23 | 345.07 | 0.3460 | -959.6 | 999999 | |
| 0.00 | 1.85 | 0.00 | 0.98 | 14.78 | 13.29 | 5.20 | 346.23 | 0.3702 | 698.0 | 536.8 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 10.63 | 12.92 | 4.84 | 344.01 | 0.3024 | 729.0 | 558.9 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 13.21 | 12.11 | 4.02 | 348.39 | 0.3408 | -631.0 | -531.8 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 15.16 | 11.83 | 3.75 | 350.17 | 0.3713 | 590.0 | 410.8 | |
| 0.00 | 1.67 | 0.00 | 0.89 | 14.77 | 11.77 | 3.68 | 350.17 | 0.3649 | -720.0 | -545.2 | |
| 0.00 | 1.67 | 0.00 | 0.87 | 11.59 | 11.50 | 3.41 | 349.20 | 0.3125 | -796.0 | -575.2 | |
| 0.00 | 1.67 | 0.00 | 0.89 | 14.29 | 11.35 | 3.27 | 351.03 | 0.3560 | -979.0 | -673.0 | |
| 0.00 | 0.44 | 0.00 | 0.23 | 12.22 | 11.20 | 3.11 | 350.46 | 0.3220 | -584.0 | -518.8 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 12.44 | 11.17 | 3.09 | 350.66 | 0.3255 | -646.0 | -478.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 11.21 | 10.88 | 2.80 | 350.92 | 0.3045 | 707.0 | 628.0 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 14.28 | 9.31 | 1.22 | 356.62 | 0.3523 | 959.0 | 756.1 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 10.86 | 7.58 | -0.51 | 1.69 | 0.2951 | 783.0 | 504.5 | |
| 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. | |