| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.86 | 22.59 | 0.61 | 16.03 | 17.40 | 99.69 | 39.02 | 303.00 | 0.7187 | 465.9 | 432.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.85 | 17.06 | 103.96 | 43.29 | 300.02 | 0.7594 | -637.0 | -527.5 | |
| 0.00 | 0.61 | 0.00 | 0.46 | 17.57 | 103.81 | 43.14 | 300.70 | 0.7604 | -498.0 | -410.7 | |
| 0.43 | 1.64 | 0.31 | 1.16 | 15.50 | 100.48 | 39.80 | 300.16 | 0.7158 | 652.4 | 518.1 | |
| 0.00 | 0.87 | 0.00 | 0.61 | 15.79 | 100.42 | 39.75 | 300.55 | 0.7168 | 475.0 | 385.9 | |
| 0.00 | 0.95 | 0.00 | 0.67 | 16.07 | 100.37 | 39.70 | 300.93 | 0.7179 | 377.0 | 285.8 | |
| 0.00 | 1.47 | 0.00 | 1.03 | 16.70 | 99.36 | 38.68 | 302.35 | 0.7110 | 577.0 | 456.5 | |
| 0.43 | 1.47 | 0.30 | 1.03 | 16.42 | 99.09 | 38.42 | 302.18 | 0.7066 | 878.0 | 738.8 | |
| 0.00 | 1.30 | 0.00 | 0.91 | 16.93 | 99.06 | 38.38 | 302.84 | 0.7093 | 545.0 | 504.3 | |
| 0.00 | 0.87 | 0.00 | 0.63 | 19.50 | 99.66 | 38.99 | 305.53 | 0.7311 | 357.0 | 296.7 | |
| 0.00 | 0.95 | 0.00 | 0.67 | 16.98 | 98.91 | 38.24 | 303.00 | 0.7082 | 729.0 | 598.7 | |
| 0.00 | 1.30 | 0.00 | 0.93 | 18.82 | 99.39 | 38.71 | 304.90 | 0.7242 | 453.0 | 471.5 | |
| 0.00 | 1.56 | 0.00 | 1.10 | 18.18 | 99.17 | 38.50 | 304.28 | 0.7181 | 420.0 | 437.4 | |
| 0.00 | 1.56 | 0.00 | 1.09 | 17.51 | 98.96 | 38.29 | 303.61 | 0.7119 | 767.0 | 643.6 | |
| 0.00 | 1.90 | 0.00 | 1.33 | 16.88 | 98.81 | 38.13 | 302.94 | 0.7064 | 786.0 | 630.6 | |
| 0.00 | 1.90 | 0.00 | 1.34 | 17.97 | 99.04 | 38.37 | 304.12 | 0.7155 | 817.0 | 590.8 | |
| 0.00 | 0.52 | 0.00 | 0.39 | 22.08 | 100.14 | 39.47 | 308.17 | 0.7515 | 316.0 | 327.0 | |
| 0.00 | 1.73 | 0.00 | 1.23 | 18.68 | 98.95 | 38.27 | 305.04 | 0.7190 | 581.0 | 552.0 | |
| 0.00 | 0.87 | 0.00 | 0.60 | 16.85 | 98.40 | 37.73 | 303.17 | 0.7021 | 610.0 | 537.3 | |
| 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. | |