| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.36 | 44.24 | 6.76 | 22.52 | 15.83 | 24.41 | 1.08 | 354.51 | 0.2290 | -162.9 | -255.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.73 | 0.00 | 0.37 | 16.26 | 29.99 | 6.66 | 334.38 | 0.2585 | -529.0 | -608.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 20.06 | 27.23 | 3.90 | 347.80 | 0.3040 | -793.0 | -712.0 | |
| 8.54 | 11.99 | 4.31 | 6.05 | 13.37 | 26.50 | 3.17 | 343.57 | 0.1912 | 1102.5 | 828.6 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 16.56 | 25.09 | 1.76 | 352.93 | 0.2397 | -753.0 | -592.0 | |
| 0.00 | 4.91 | 0.00 | 2.50 | 16.31 | 24.80 | 1.47 | 353.96 | 0.2349 | -1126.0 | -907.0 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 15.90 | 24.67 | 1.34 | 354.31 | 0.2278 | -1042.0 | -845.6 | |
| 0.00 | 2.45 | 0.00 | 1.24 | 14.40 | 24.44 | 1.11 | 354.65 | 0.2019 | -1181.0 | -903.1 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 13.47 | 24.18 | 0.85 | 355.50 | 0.1856 | 822.0 | 588.1 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 22.87 | 24.16 | 0.83 | 357.75 | 0.3439 | -723.0 | -499.9 | |
| 3.18 | 6.27 | 1.61 | 3.18 | 15.37 | 24.09 | 0.77 | 356.59 | 0.2180 | -1033.0 | -557.6 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 15.34 | 23.87 | 0.54 | 357.57 | 0.2172 | -826.0 | -645.7 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 16.90 | 23.37 | 0.04 | 359.84 | 0.2438 | -993.0 | -835.6 | |
| 0.00 | 3.09 | 0.00 | 1.58 | 17.47 | 22.63 | -0.70 | 2.63 | 0.2536 | -701.0 | -643.4 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 18.01 | 21.41 | -1.92 | 6.94 | 0.2644 | 833.0 | 671.7 | |
| 1.64 | 5.72 | 0.84 | 2.93 | 17.59 | 20.84 | -2.49 | 9.24 | 0.2589 | 1033.2 | 863.2 | |
| 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. | |