| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.72 | 0.00 | 11.41 | 5.26 | 260.56 | -29.86 | 84.94 | 0.4982 | 379.9 | 381.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.82 | 0.00 | 0.41 | 1.70 | 279.46 | -10.96 | 97.07 | 0.1923 | -477.0 | -527.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 3.40 | 278.45 | -11.97 | 88.27 | 0.2080 | -756.0 | -646.1 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 0.81 | 278.28 | -12.14 | 100.50 | 0.2147 | -714.0 | -604.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 11.02 | 267.89 | -22.53 | 69.36 | 0.4035 | 684.0 | 599.3 | |
| 0.00 | 2.18 | 0.00 | 1.21 | 9.77 | 264.34 | -26.07 | 74.33 | 0.4516 | 815.0 | 605.3 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 8.72 | 261.22 | -29.19 | 77.77 | 0.4952 | 828.0 | 616.6 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 8.44 | 261.17 | -29.24 | 78.34 | 0.4953 | 589.0 | 555.7 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -4.11 | 258.36 | -32.05 | 102.50 | 0.5442 | 616.0 | 460.2 | |
| 0.00 | 0.91 | 0.00 | 0.53 | -1.19 | 258.42 | -31.99 | 97.19 | 0.5360 | 637.0 | 570.4 | |
| 0.00 | 3.45 | 0.00 | 2.02 | 4.39 | 258.22 | -32.19 | 86.70 | 0.5341 | 688.0 | 483.6 | |
| 0.00 | 1.82 | 0.00 | 1.07 | 7.76 | 257.60 | -32.82 | 80.52 | 0.5465 | 682.0 | 554.7 | |
| 0.00 | 1.18 | 0.00 | 0.76 | 5.53 | 250.76 | -39.65 | 85.08 | 0.6398 | 664.0 | 491.5 | |
| 0.00 | 0.73 | 0.00 | 0.47 | 5.74 | 249.74 | -40.67 | 84.80 | 0.6534 | 564.0 | 482.8 | |
| 0.00 | 0.73 | 0.00 | 0.48 | 2.68 | 249.52 | -40.89 | 89.50 | 0.6562 | 235.0 | 196.2 | |
| 0.00 | 1.09 | 0.00 | 0.72 | 4.37 | 248.94 | -41.47 | 86.92 | 0.6635 | 643.0 | 597.2 | |
| 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. | |