| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.99 | 0.00 | 13.55 | -8.41 | 8.76 | 17.74 | 261.70 | 0.3066 | 378.2 | 302.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.42 | -8.04 | 11.40 | 20.38 | 263.44 | 0.3487 | 690.0 | 535.6 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -8.16 | 11.35 | 20.32 | 263.08 | 0.3479 | 854.0 | 645.0 | |
| 0.00 | 1.59 | 0.00 | 0.84 | -8.22 | 11.16 | 20.13 | 262.84 | 0.3448 | 929.0 | 785.3 | |
| 0.00 | 2.73 | 0.00 | 1.44 | -8.53 | 11.04 | 20.02 | 261.93 | 0.3435 | 967.0 | 790.8 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -9.14 | 10.62 | 19.60 | 259.99 | 0.3378 | 799.0 | 650.7 | |
| 0.00 | 1.59 | 0.00 | 0.83 | -9.12 | 10.43 | 19.41 | 259.98 | 0.3346 | 810.0 | 712.6 | |
| 0.00 | 1.76 | 0.00 | 0.93 | -8.82 | 10.38 | 19.36 | 260.86 | 0.3332 | 798.0 | 703.5 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -7.67 | 9.68 | 18.66 | 264.19 | 0.3201 | 386.0 | 415.0 | |
| 0.00 | 1.50 | 0.00 | 0.78 | -7.69 | 9.17 | 18.15 | 264.03 | 0.3118 | 684.0 | 568.8 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -10.53 | 8.87 | 17.85 | 254.87 | 0.3135 | 782.0 | 620.8 | |
| 0.00 | 2.47 | 0.00 | 1.29 | -10.08 | 8.84 | 17.82 | 256.27 | 0.3116 | 647.0 | 633.1 | |
| 0.00 | 1.23 | 0.00 | 0.64 | -9.93 | 8.74 | 17.72 | 256.67 | 0.3094 | 574.0 | 542.6 | |
| 0.00 | 1.15 | 0.00 | 0.59 | -3.86 | 7.82 | 16.80 | 276.98 | 0.2918 | 622.0 | 435.1 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -7.42 | 6.07 | 15.04 | 264.25 | 0.2599 | -893.0 | -780.1 | |
| 0.00 | 1.32 | 0.00 | 0.68 | -7.61 | 5.67 | 14.64 | 263.39 | 0.2534 | -782.0 | -688.7 | |
| 0.00 | 2.38 | 0.00 | 1.22 | -7.34 | 5.66 | 14.63 | 264.45 | 0.2529 | -766.0 | -615.7 | |
| 0.00 | 2.11 | 0.00 | 1.08 | -8.11 | 5.03 | 14.00 | 261.12 | 0.2436 | -672.0 | -596.5 | |
| 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. | |