| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.49 | 172.84 | 24.88 | 150.58 | 23.41 | 302.62 | 55.02 | 293.75 | 0.8214 | -54.0 | -89.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.25 | 125.91 | 15.79 | 115.46 | 22.68 | 305.02 | 57.42 | 292.37 | 0.8428 | -829.2 | -229.2 | |
| 0.00 | 1.52 | 0.00 | 1.33 | 23.02 | 303.26 | 55.66 | 293.00 | 0.8277 | -563.0 | -458.2 | |
| 3.40 | 6.70 | 2.54 | 5.02 | 25.06 | 295.04 | 47.43 | 297.21 | 0.7525 | 483.6 | 215.4 | |
| 0.00 | 3.13 | 0.00 | 2.36 | 25.65 | 295.35 | 47.74 | 297.89 | 0.7571 | 409.0 | 357.6 | |
| 0.89 | 1.97 | 0.67 | 1.48 | 25.51 | 295.07 | 47.47 | 297.79 | 0.7540 | 668.5 | 598.2 | |
| 0.00 | 1.34 | 0.00 | 1.01 | 25.79 | 294.87 | 47.26 | 298.21 | 0.7527 | 505.0 | 408.5 | |
| 0.00 | 1.43 | 0.00 | 1.07 | 25.72 | 294.54 | 46.93 | 298.21 | 0.7492 | 541.0 | 467.1 | |
| 3.75 | 7.51 | 2.82 | 5.65 | 26.58 | 294.84 | 47.24 | 299.23 | 0.7547 | 656.3 | 391.4 | |
| 0.00 | 3.75 | 0.00 | 2.78 | 25.85 | 294.26 | 46.65 | 298.46 | 0.7467 | 786.0 | 578.0 | |
| 0.00 | 4.83 | 0.00 | 3.56 | 25.48 | 293.97 | 46.37 | 298.06 | 0.7427 | 722.0 | 656.1 | |
| 0.00 | 1.97 | 0.00 | 1.45 | 25.78 | 293.83 | 46.23 | 298.50 | 0.7422 | 767.0 | 670.4 | |
| 2.68 | 3.13 | 1.95 | 2.28 | 25.21 | 293.35 | 45.75 | 297.89 | 0.7356 | 666.8 | 634.4 | |
| 0.00 | 4.02 | 0.00 | 2.97 | 26.25 | 293.78 | 46.17 | 299.12 | 0.7430 | 586.0 | 514.0 | |
| 0.00 | 1.16 | 0.00 | 0.89 | 28.94 | 295.03 | 47.43 | 302.17 | 0.7637 | 475.0 | 434.3 | |
| 0.00 | 1.61 | 0.00 | 1.19 | 26.88 | 293.57 | 45.97 | 300.02 | 0.7429 | 672.0 | 572.2 | |
| 0.00 | 0.89 | 0.00 | 0.65 | 26.04 | 293.14 | 45.53 | 299.06 | 0.7358 | 680.0 | 622.3 | |
| 1.52 | 1.97 | 1.11 | 1.43 | 26.31 | 293.08 | 45.47 | 299.43 | 0.7360 | 673.9 | 650.2 | |
| 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. | |