| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.67 | 0.00 | 9.79 | 12.37 | 257.25 | -31.50 | 74.96 | 0.5326 | 484.3 | 385.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.44 | 16.31 | 268.77 | -19.98 | 59.84 | 0.3809 | -773.0 | -604.7 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 16.08 | 268.66 | -20.09 | 60.48 | 0.3808 | -679.0 | -579.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 16.43 | 259.17 | -29.58 | 67.18 | 0.5158 | 735.0 | 565.5 | |
| 0.00 | 1.36 | 0.00 | 0.79 | 16.42 | 258.40 | -30.35 | 67.59 | 0.5263 | 710.0 | 480.1 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 8.43 | 259.19 | -29.56 | 82.85 | 0.4938 | 848.0 | 693.6 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 8.13 | 259.18 | -29.57 | 83.48 | 0.4937 | 651.0 | 540.3 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 8.61 | 259.00 | -29.75 | 82.53 | 0.4969 | 780.0 | 617.8 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 9.70 | 258.22 | -30.53 | 80.47 | 0.5098 | 609.0 | 469.0 | |
| 0.00 | 1.09 | 0.00 | 0.65 | 19.38 | 256.12 | -32.63 | 63.65 | 0.5698 | 639.0 | 485.1 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 16.58 | 255.83 | -32.92 | 68.55 | 0.5618 | 343.0 | 365.9 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 10.61 | 255.56 | -33.19 | 79.25 | 0.5497 | 763.0 | 582.8 | |
| 0.00 | 0.72 | 0.00 | 0.43 | 2.34 | 255.03 | -33.72 | 94.26 | 0.5583 | 598.0 | 492.5 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 5.06 | 254.55 | -34.20 | 89.33 | 0.5621 | 838.0 | 682.9 | |
| 0.00 | 0.72 | 0.00 | 0.47 | 19.53 | 249.57 | -39.18 | 66.36 | 0.6522 | 615.0 | 500.9 | |
| 0.00 | 1.72 | 0.00 | 1.15 | 11.20 | 246.72 | -42.03 | 79.52 | 0.6702 | 588.0 | 388.6 | |
| 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. | |