| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.04 | 55.53 | 0.61 | 31.54 | 9.17 | 121.49 | 22.39 | 309.48 | 0.4791 | -212.1 | -267.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.71 | 4.40 | 129.90 | 30.80 | 289.81 | 0.5448 | -751.0 | -599.4 | |
| 0.00 | 1.47 | 0.00 | 0.86 | 4.24 | 129.72 | 30.62 | 289.65 | 0.5415 | -767.0 | -629.1 | |
| 0.00 | 0.95 | 0.00 | 0.58 | 10.22 | 130.19 | 31.09 | 299.03 | 0.5834 | -708.0 | -469.6 | |
| 0.00 | 1.73 | 0.00 | 1.02 | 4.44 | 129.56 | 30.46 | 290.10 | 0.5403 | -726.0 | -683.7 | |
| 0.00 | 0.78 | 0.00 | 0.46 | 5.81 | 129.60 | 30.50 | 292.42 | 0.5483 | -582.0 | -423.2 | |
| 0.00 | 1.47 | 0.00 | 0.87 | 6.01 | 129.30 | 30.20 | 292.96 | 0.5454 | -855.0 | -590.7 | |
| 0.00 | 0.86 | 0.00 | 0.51 | 7.14 | 129.38 | 30.28 | 294.80 | 0.5532 | -608.0 | -479.6 | |
| 0.00 | 1.04 | 0.00 | 0.63 | 10.15 | 129.55 | 30.44 | 299.44 | 0.5749 | -666.0 | -514.8 | |
| 0.00 | 2.07 | 0.00 | 1.22 | 6.39 | 129.05 | 29.94 | 293.79 | 0.5443 | -858.0 | -643.8 | |
| 0.00 | 2.59 | 0.00 | 1.52 | 6.19 | 128.89 | 29.79 | 293.58 | 0.5411 | -943.0 | -787.4 | |
| 1.04 | 3.37 | 0.61 | 1.98 | 6.71 | 128.79 | 29.69 | 294.52 | 0.5428 | -865.1 | -690.3 | |
| 0.00 | 0.95 | 0.00 | 0.57 | 9.71 | 129.05 | 29.94 | 299.18 | 0.5657 | -595.0 | -509.4 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 8.31 | 128.91 | 29.81 | 297.07 | 0.5546 | -629.0 | -544.6 | |
| 0.00 | 2.68 | 0.00 | 1.60 | 8.95 | 128.83 | 29.73 | 298.17 | 0.5579 | -713.0 | -566.5 | |
| 0.00 | 2.16 | 0.00 | 1.29 | 9.29 | 128.80 | 29.69 | 298.73 | 0.5597 | -735.0 | -598.2 | |
| 0.00 | 1.38 | 0.00 | 0.82 | 9.40 | 128.60 | 29.50 | 299.07 | 0.5580 | -773.0 | -712.5 | |
| 0.00 | 1.55 | 0.00 | 0.92 | 8.83 | 128.34 | 29.24 | 298.38 | 0.5507 | -892.0 | -697.6 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 9.38 | 127.66 | 28.56 | 299.84 | 0.5460 | 594.0 | 452.4 | |
| 0.00 | 1.47 | 0.00 | 0.83 | 11.72 | 121.60 | 22.50 | 310.08 | 0.4917 | -705.0 | -565.2 | |
| 0.00 | 0.78 | 0.00 | 0.45 | 14.06 | 121.07 | 21.97 | 314.31 | 0.5092 | -678.0 | -542.6 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 13.61 | 120.89 | 21.79 | 313.89 | 0.5026 | -538.0 | -486.3 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 13.32 | 120.20 | 21.10 | 314.38 | 0.4922 | -822.0 | -706.9 | |
| 0.00 | 1.21 | 0.00 | 0.69 | 13.54 | 120.16 | 21.06 | 314.76 | 0.4940 | -791.0 | -620.4 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 17.28 | 120.23 | 21.13 | 319.75 | 0.5350 | -633.0 | -542.9 | |
| 0.00 | 1.90 | 0.00 | 1.07 | 13.22 | 119.35 | 20.25 | 315.42 | 0.4819 | -578.0 | -595.4 | |
| 0.00 | 3.80 | 0.00 | 2.14 | 12.98 | 118.97 | 19.87 | 315.60 | 0.4753 | -685.0 | -799.9 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 8.18 | 112.03 | 12.93 | 319.84 | 0.3450 | 899.0 | 703.7 | |
| 0.00 | 1.99 | 0.00 | 1.04 | 8.21 | 110.84 | 11.74 | 322.63 | 0.3331 | 821.0 | 720.7 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 8.20 | 110.56 | 11.46 | 323.27 | 0.3303 | 724.0 | 625.2 | |
| 0.00 | 0.95 | 0.00 | 0.50 | 8.63 | 110.54 | 11.44 | 324.09 | 0.3359 | 755.0 | 565.1 | |
| 0.00 | 2.25 | 0.00 | 1.18 | 8.79 | 109.45 | 10.35 | 327.06 | 0.3279 | 958.0 | 776.0 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 8.38 | 107.24 | 8.14 | 332.38 | 0.3036 | 871.0 | 642.7 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 8.28 | 107.06 | 7.96 | 332.77 | 0.3007 | 1028.0 | 923.2 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 12.20 | 106.55 | 7.45 | 339.09 | 0.3566 | 665.0 | 398.6 | |
| 0.00 | 1.38 | 0.00 | 0.72 | 10.68 | 102.80 | 3.70 | 348.34 | 0.3152 | 847.0 | 733.3 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 10.15 | 101.92 | 2.82 | 350.79 | 0.3037 | 839.0 | 664.2 | |
| 0.00 | 1.55 | 0.00 | 0.81 | 10.08 | 101.71 | 2.60 | 351.45 | 0.3021 | 991.0 | 826.7 | |
| 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. | |