| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.25 | 32.26 | 0.63 | 16.25 | 16.78 | 327.40 | 0.54 | 327.62 | 0.1828 | 96.4 | 172.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.45 | 12.85 | 334.38 | 7.52 | 308.26 | 0.1633 | -870.0 | -761.7 | |
| 0.00 | 2.33 | 0.00 | 1.17 | 15.80 | 332.87 | 6.01 | 326.37 | 0.1826 | -890.0 | -624.9 | |
| 0.00 | 1.88 | 0.00 | 0.95 | 17.68 | 332.64 | 5.78 | 332.41 | 0.2081 | -795.0 | -723.0 | |
| 0.00 | 1.79 | 0.00 | 0.91 | 17.62 | 332.29 | 5.43 | 333.72 | 0.2045 | -1021.0 | -779.4 | |
| 0.00 | 2.42 | 0.00 | 1.23 | 19.53 | 329.29 | 2.43 | 349.46 | 0.2194 | -1107.0 | -816.5 | |
| 1.25 | 5.20 | 0.63 | 2.62 | 17.31 | 328.50 | 1.64 | 351.22 | 0.1796 | 984.8 | 812.0 | |
| 0.00 | 3.49 | 0.00 | 1.75 | 16.12 | 327.42 | 0.56 | 356.58 | 0.1571 | 491.0 | 456.2 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 19.26 | 327.33 | 0.47 | 357.89 | 0.2111 | -934.0 | -700.2 | |
| 0.00 | 3.67 | 0.00 | 1.84 | 16.30 | 326.82 | -0.04 | 0.25 | 0.1600 | 929.0 | 785.7 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 17.07 | 326.53 | -0.33 | 1.81 | 0.1734 | 839.0 | 718.1 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 16.15 | 326.41 | -0.45 | 2.77 | 0.1576 | 829.0 | 644.1 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 15.90 | 326.25 | -0.61 | 3.83 | 0.1535 | 888.0 | 753.8 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 14.86 | 321.68 | -5.18 | 32.90 | 0.1615 | 796.0 | 484.6 | |
| 0.00 | 2.33 | 0.00 | 1.19 | 18.62 | 319.97 | -6.89 | 29.63 | 0.2311 | 1041.0 | 841.0 | |
| 0.00 | 2.69 | 0.00 | 1.35 | 13.62 | 319.73 | -7.13 | 46.64 | 0.1666 | 594.0 | 441.4 | |
| 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. | |