| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.16 | 153.14 | 22.51 | 130.46 | 13.36 | 117.03 | 54.27 | 283.70 | 0.8147 | -459.3 | -199.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.69 | 131.65 | 21.40 | 114.15 | 13.83 | 117.75 | 54.99 | 284.22 | 0.8226 | -911.2 | -246.9 | |
| 0.00 | 1.21 | 0.00 | 0.98 | 9.94 | 115.37 | 52.61 | 279.60 | 0.7960 | -556.0 | -476.6 | |
| 0.00 | 0.26 | 0.00 | 0.22 | 13.80 | 116.11 | 53.34 | 284.36 | 0.8064 | -605.0 | -494.0 | |
| 0.00 | 1.38 | 0.00 | 1.09 | 12.28 | 113.79 | 51.03 | 282.71 | 0.7811 | 261.0 | 199.7 | |
| 1.47 | 7.77 | 1.11 | 5.90 | 8.01 | 112.15 | 49.39 | 277.28 | 0.7602 | -722.2 | -537.7 | |
| 0.00 | 1.04 | 0.00 | 0.80 | 12.66 | 112.89 | 50.12 | 283.31 | 0.7717 | 412.0 | 317.9 | |
| 0.00 | 0.86 | 0.00 | 0.66 | 12.04 | 112.63 | 49.86 | 282.53 | 0.7683 | 474.0 | 334.5 | |
| 0.00 | 2.07 | 0.00 | 1.58 | 11.82 | 112.24 | 49.48 | 282.29 | 0.7638 | 682.0 | 599.2 | |
| 0.00 | 1.21 | 0.00 | 0.91 | 12.28 | 111.47 | 48.71 | 282.99 | 0.7557 | 597.0 | 491.0 | |
| 0.00 | 1.12 | 0.00 | 0.83 | 12.29 | 110.60 | 47.84 | 283.12 | 0.7460 | 510.0 | 498.2 | |
| 0.00 | 1.29 | 0.00 | 0.95 | 10.48 | 110.10 | 47.34 | 280.74 | 0.7384 | 661.0 | 582.4 | |
| 0.00 | 0.95 | 0.00 | 0.70 | 10.84 | 110.13 | 47.37 | 281.22 | 0.7391 | 699.0 | 583.4 | |
| 0.00 | 0.78 | 0.00 | 0.57 | 11.20 | 110.12 | 47.36 | 281.71 | 0.7393 | 657.0 | 582.4 | |
| 0.00 | 1.55 | 0.00 | 1.12 | 8.09 | 109.37 | 46.61 | 277.53 | 0.7280 | 658.0 | 606.1 | |
| 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. | |