| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.50 | 142.85 | 19.06 | 78.73 | 6.31 | 204.70 | 25.68 | 276.40 | 0.4354 | -387.9 | -189.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.63 | 0.00 | 1.47 | 4.26 | 206.58 | 27.56 | 271.60 | 0.4634 | -923.0 | -735.9 | |
| 16.79 | 74.44 | 9.36 | 41.50 | 5.89 | 206.27 | 27.25 | 275.15 | 0.4592 | -1035.8 | -330.1 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 5.31 | 206.00 | 26.98 | 273.92 | 0.4547 | -813.0 | -661.9 | |
| 6.17 | -2.00 | 3.43 | -2.00 | 5.87 | 205.82 | 26.80 | 275.17 | 0.4523 | -1174.9 | 999999 | |
| 0.00 | 2.27 | 0.00 | 1.26 | 4.90 | 205.67 | 26.65 | 273.01 | 0.4494 | -716.0 | -581.6 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 3.32 | 205.34 | 26.32 | 269.47 | 0.4445 | -906.0 | -715.7 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 10.09 | 205.72 | 26.70 | 284.45 | 0.4586 | -721.0 | -646.7 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 4.79 | 205.23 | 26.20 | 272.79 | 0.4424 | -782.0 | -693.1 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 9.89 | 205.52 | 26.50 | 284.08 | 0.4551 | -884.0 | -623.4 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 4.83 | 205.06 | 26.04 | 272.87 | 0.4397 | -790.0 | -626.8 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 6.84 | 205.09 | 26.07 | 277.45 | 0.4419 | -795.0 | -676.7 | |
| 0.00 | 2.09 | 0.00 | 1.15 | 3.10 | 204.79 | 25.77 | 268.90 | 0.4360 | -672.0 | -386.7 | |
| 0.54 | 2.00 | 0.30 | 1.10 | 7.79 | 204.84 | 25.82 | 279.67 | 0.4396 | 692.5 | 600.9 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 5.84 | 204.70 | 25.67 | 275.24 | 0.4346 | -731.0 | -664.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | 3.59 | 204.57 | 25.55 | 270.02 | 0.4322 | -828.0 | -642.8 | |
| 0.00 | 1.72 | 0.00 | 0.96 | 13.62 | 205.22 | 26.20 | 292.14 | 0.4651 | -817.0 | -649.5 | |
| 0.00 | 1.72 | 0.00 | 0.95 | 6.95 | 204.48 | 25.46 | 277.83 | 0.4326 | -852.0 | -573.4 | |
| 0.82 | 3.00 | 0.45 | 1.64 | 6.26 | 204.11 | 25.09 | 276.29 | 0.4258 | -867.2 | -719.9 | |
| 0.00 | 0.54 | 0.00 | 0.30 | 7.48 | 204.18 | 25.16 | 279.13 | 0.4286 | -742.0 | -568.2 | |
| 0.00 | 2.90 | 0.00 | 1.59 | 8.27 | 204.20 | 25.17 | 280.96 | 0.4306 | 396.0 | 361.8 | |
| 3.09 | 4.45 | 1.69 | 2.44 | 8.49 | 204.14 | 25.12 | 281.48 | 0.4302 | 843.0 | 543.8 | |
| 0.00 | 3.90 | 0.00 | 2.14 | 8.13 | 203.98 | 24.96 | 280.69 | 0.4269 | 289.0 | 437.6 | |
| 2.00 | 3.18 | 1.09 | 1.73 | 6.18 | 203.73 | 24.71 | 276.16 | 0.4197 | -949.3 | -739.7 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 7.92 | 203.56 | 24.54 | 280.36 | 0.4199 | 721.0 | 564.4 | |
| 1.91 | 3.90 | 1.04 | 2.13 | 8.11 | 203.47 | 24.45 | 280.83 | 0.4189 | 1061.8 | 849.2 | |
| 1.09 | 2.36 | 0.59 | 1.28 | 6.35 | 203.00 | 23.98 | 276.71 | 0.4084 | -980.5 | -813.9 | |
| 0.00 | 2.09 | 0.00 | 1.13 | 6.48 | 202.80 | 23.78 | 277.06 | 0.4054 | -757.0 | -536.6 | |
| 1.00 | 3.63 | 0.54 | 1.96 | 7.10 | 202.50 | 23.48 | 278.67 | 0.4016 | 909.9 | 649.3 | |
| 0.45 | 2.81 | 0.24 | 1.51 | 6.66 | 201.88 | 22.86 | 277.72 | 0.3910 | 894.2 | 708.7 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 5.85 | 200.35 | 21.33 | 275.91 | 0.3653 | 775.0 | 653.4 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 9.83 | 199.81 | 20.79 | 286.96 | 0.3671 | 650.0 | 557.5 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 6.25 | 197.72 | 18.70 | 277.75 | 0.3231 | 737.0 | 697.2 | |
| 0.00 | 2.72 | 0.00 | 1.42 | 6.52 | 197.67 | 18.65 | 278.62 | 0.3227 | 775.0 | 693.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 6.21 | 196.46 | 17.44 | 278.08 | 0.3023 | 891.0 | 697.0 | |
| 0.64 | 2.00 | 0.33 | 1.04 | 6.40 | 196.37 | 17.35 | 278.73 | 0.3012 | 1035.6 | 878.7 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 5.63 | 192.09 | 13.07 | 277.77 | 0.2282 | -961.0 | -679.1 | |
| 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. | |