| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.11 | 192.18 | 17.44 | 101.53 | 19.67 | 103.65 | -6.01 | 16.63 | 0.3463 | -824.6 | -405.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.61 | 24.76 | 104.73 | -4.93 | 10.72 | 0.4219 | -723.0 | -620.4 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 22.13 | 104.47 | -5.19 | 12.74 | 0.3815 | -692.0 | -574.0 | |
| 31.66 | 166.94 | 16.63 | 87.71 | 19.01 | 103.95 | -5.71 | 16.41 | 0.3345 | -1289.9 | -417.4 | |
| 0.00 | 2.05 | 0.00 | 1.13 | 25.48 | 103.48 | -6.18 | 12.91 | 0.4370 | -800.0 | -726.8 | |
| 0.00 | 1.28 | 0.00 | 0.69 | 23.18 | 103.53 | -6.13 | 14.22 | 0.4015 | -874.0 | -723.1 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 19.76 | 103.45 | -6.21 | 17.06 | 0.3486 | -576.0 | -375.4 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 28.49 | 102.74 | -6.92 | 12.68 | 0.4849 | -532.0 | -450.1 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 26.00 | 102.76 | -6.90 | 14.03 | 0.4476 | -749.0 | -593.8 | |
| 0.00 | 0.68 | 0.00 | 0.38 | 26.20 | 101.85 | -7.81 | 15.64 | 0.4542 | -782.0 | -732.2 | |
| 0.00 | 1.96 | 0.00 | 1.09 | 25.93 | 101.70 | -7.96 | 16.10 | 0.4509 | -920.0 | -704.8 | |
| 1.45 | 3.67 | 0.81 | 2.04 | 26.23 | 101.55 | -8.11 | 16.19 | 0.4559 | -801.9 | -698.7 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 25.34 | 101.48 | -8.18 | 16.95 | 0.4431 | -789.0 | -607.5 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 15.67 | 101.40 | -8.26 | 27.69 | 0.2992 | 890.0 | 683.0 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 26.82 | 100.74 | -8.93 | 17.27 | 0.4683 | -664.0 | -612.6 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 17.86 | 99.95 | -9.71 | 28.13 | 0.3421 | 827.0 | 635.1 | |
| 0.00 | 1.19 | 0.00 | 0.69 | 29.26 | 98.54 | -11.13 | 19.22 | 0.5136 | -726.0 | -581.9 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 18.44 | 99.16 | -10.51 | 29.15 | 0.3567 | 669.0 | 571.8 | |
| 0.00 | 1.96 | 0.00 | 1.04 | 18.26 | 99.14 | -10.53 | 29.47 | 0.3542 | 965.0 | 814.1 | |
| 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. | |