| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 58.04 | 0.00 | 31.77 | 9.98 | 171.95 | 24.26 | 281.85 | 0.4138 | 289.7 | 378.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.71 | 6.75 | 183.05 | 35.36 | 272.67 | 0.5775 | -634.0 | -540.8 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 11.93 | 180.35 | 32.66 | 282.17 | 0.5423 | -855.0 | -631.4 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 5.84 | 179.59 | 31.90 | 270.78 | 0.5279 | -744.0 | -698.4 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 12.55 | 180.29 | 32.60 | 283.32 | 0.5425 | -726.0 | -670.8 | |
| 0.00 | 0.45 | 0.00 | 0.26 | 11.30 | 180.04 | 32.36 | 281.07 | 0.5369 | -646.0 | -532.6 | |
| 0.00 | 0.72 | 0.00 | 0.42 | 13.02 | 180.02 | 32.34 | 284.26 | 0.5398 | -479.0 | -445.1 | |
| 0.00 | 0.54 | 0.00 | 0.32 | 8.95 | 179.49 | 31.80 | 276.72 | 0.5262 | -713.0 | -593.3 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 11.49 | 178.90 | 31.21 | 281.67 | 0.5206 | -738.0 | -585.8 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 8.79 | 178.57 | 30.88 | 276.48 | 0.5125 | -672.0 | -594.6 | |
| 0.00 | 1.26 | 0.00 | 0.73 | 11.34 | 178.34 | 30.65 | 281.50 | 0.5121 | -778.0 | -597.6 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 9.17 | 177.82 | 30.13 | 277.30 | 0.5016 | -798.0 | -643.6 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 12.17 | 177.76 | 30.07 | 283.27 | 0.5052 | -711.0 | -603.1 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 9.57 | 175.59 | 27.91 | 278.42 | 0.4685 | -707.0 | -552.9 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 10.01 | 174.66 | 26.97 | 279.56 | 0.4548 | 733.0 | 471.6 | |
| 0.00 | 2.08 | 0.00 | 1.15 | 10.12 | 174.29 | 26.60 | 279.88 | 0.4493 | 848.0 | 678.8 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 10.47 | 174.11 | 26.43 | 280.69 | 0.4472 | 738.0 | 597.9 | |
| 0.00 | 0.81 | 0.00 | 0.45 | 10.42 | 173.77 | 26.08 | 280.69 | 0.4418 | 919.0 | 765.2 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 9.76 | 173.50 | 25.81 | 279.25 | 0.4366 | 707.0 | 580.1 | |
| 0.00 | 5.24 | 0.00 | 2.87 | 9.08 | 173.14 | 25.45 | 277.75 | 0.4300 | 929.0 | 752.0 | |
| 0.00 | 3.43 | 0.00 | 1.88 | 8.57 | 173.07 | 25.38 | 276.56 | 0.4284 | 758.0 | 666.7 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 8.81 | 173.05 | 25.36 | 277.13 | 0.4284 | 863.0 | 725.9 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 9.30 | 173.05 | 25.37 | 278.27 | 0.4290 | 899.0 | 845.9 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 9.58 | 172.94 | 25.25 | 278.95 | 0.4276 | 787.0 | 615.7 | |
| 0.00 | 2.35 | 0.00 | 1.29 | 9.89 | 172.86 | 25.17 | 279.69 | 0.4269 | 675.0 | 598.5 | |
| 0.00 | 2.53 | 0.00 | 1.38 | 8.95 | 172.69 | 25.00 | 277.52 | 0.4228 | 798.0 | 652.5 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 8.04 | 172.62 | 24.93 | 275.36 | 0.4210 | 709.0 | 541.5 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 9.35 | 172.58 | 24.89 | 278.49 | 0.4217 | 775.0 | 679.3 | |
| 0.00 | 1.99 | 0.00 | 1.08 | 9.33 | 172.37 | 24.69 | 278.48 | 0.4184 | 946.0 | 737.3 | |
| 0.00 | 4.43 | 0.00 | 2.41 | 9.00 | 172.25 | 24.56 | 277.71 | 0.4160 | 671.0 | 674.1 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 7.36 | 167.86 | 20.17 | 273.99 | 0.3443 | 798.0 | 647.3 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 7.80 | 166.00 | 18.31 | 275.55 | 0.3141 | 679.0 | 478.0 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 12.57 | 165.44 | 17.75 | 290.80 | 0.3197 | 889.0 | 695.1 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 11.14 | 162.37 | 14.68 | 289.19 | 0.2645 | 894.0 | 682.8 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 7.84 | 161.75 | 14.06 | 276.81 | 0.2435 | 734.0 | 595.0 | |
| 0.00 | 2.08 | 0.00 | 1.05 | 11.76 | 158.36 | 10.68 | 297.81 | 0.2060 | 966.0 | 765.5 | |
| 0.00 | 2.08 | 0.00 | 1.06 | 14.06 | 158.24 | 10.56 | 307.31 | 0.2244 | 881.0 | 729.0 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 13.86 | 157.69 | 10.01 | 307.99 | 0.2150 | 802.0 | 671.2 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 13.70 | 156.07 | 8.38 | 312.24 | 0.1922 | 811.0 | 626.9 | |
| 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. | |