| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.58 | 388.88 | 37.90 | 228.84 | 16.15 | 110.40 | -29.47 | 61.21 | 0.5410 | -874.3 | -322.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.24 | 375.87 | 37.69 | 220.65 | 16.15 | 110.63 | -29.24 | 61.08 | 0.5381 | -1420.7 | -361.3 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 15.49 | 108.38 | -31.48 | 63.73 | 0.5634 | 736.0 | 561.0 | |
| 0.34 | 1.28 | 0.21 | 0.79 | 17.04 | 106.82 | -33.04 | 62.21 | 0.5916 | 779.0 | 664.3 | |
| 0.00 | 0.86 | 0.00 | 0.52 | 16.42 | 106.90 | -32.96 | 63.13 | 0.5873 | 613.0 | 539.1 | |
| 0.00 | 1.11 | 0.00 | 0.69 | 16.13 | 105.36 | -34.50 | 64.48 | 0.6052 | 813.0 | 667.4 | |
| 0.00 | 0.60 | 0.00 | 0.37 | 16.47 | 105.26 | -34.61 | 64.01 | 0.6082 | 695.0 | 600.6 | |
| 0.00 | 1.71 | 0.00 | 1.07 | 16.06 | 104.70 | -35.16 | 64.94 | 0.6132 | 697.0 | 509.2 | |
| 0.00 | 0.86 | 0.00 | 0.54 | 17.03 | 103.84 | -36.02 | 63.91 | 0.6283 | 544.0 | 486.9 | |
| 0.00 | 1.28 | 0.00 | 0.82 | 16.76 | 103.68 | -36.19 | 64.41 | 0.6291 | 739.0 | 565.5 | |
| 0.00 | 0.26 | 0.00 | 0.16 | 16.38 | 102.72 | -37.14 | 65.46 | 0.6392 | 659.0 | 687.3 | |
| 0.00 | 0.68 | 0.00 | 0.44 | 16.62 | 102.39 | -37.47 | 65.26 | 0.6442 | 618.0 | 519.2 | |
| 0.00 | 1.03 | 0.00 | 0.66 | 15.88 | 102.25 | -37.62 | 66.42 | 0.6429 | 691.0 | 613.2 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 15.84 | 101.90 | -37.96 | 66.62 | 0.6470 | 698.0 | 567.4 | |
| 0.00 | 1.80 | 0.00 | 1.17 | 15.60 | 101.68 | -38.18 | 67.09 | 0.6487 | 600.0 | 495.2 | |
| 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. | |