| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.62 | 38.33 | 6.44 | 19.58 | 15.96 | 24.11 | 4.62 | 340.63 | 0.2442 | -61.1 | -243.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.52 | 19.98 | 27.22 | 7.73 | 336.76 | 0.3219 | -830.0 | -637.4 | |
| 5.45 | 8.99 | 2.77 | 4.57 | 13.42 | 26.67 | 7.18 | 326.46 | 0.2210 | 1102.1 | 777.5 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 15.64 | 25.18 | 5.69 | 336.64 | 0.2420 | -988.0 | -768.0 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 16.05 | 25.16 | 5.67 | 337.39 | 0.2482 | -741.0 | -625.8 | |
| 1.45 | 5.54 | 0.74 | 2.84 | 16.36 | 25.01 | 5.52 | 338.41 | 0.2521 | -964.9 | -488.0 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 15.49 | 24.51 | 5.02 | 338.89 | 0.2353 | -1124.0 | -903.9 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.77 | 24.45 | 4.97 | 339.54 | 0.2394 | -667.0 | -635.0 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 14.59 | 24.39 | 4.90 | 337.83 | 0.2203 | -905.0 | -726.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 16.68 | 24.41 | 4.93 | 340.99 | 0.2536 | -813.0 | -545.9 | |
| 0.00 | 2.82 | 0.00 | 1.44 | 16.56 | 23.61 | 4.13 | 343.75 | 0.2476 | -937.0 | -765.5 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 18.33 | 21.41 | 1.92 | 353.20 | 0.2695 | -807.0 | -593.2 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 17.45 | 21.24 | 1.75 | 353.40 | 0.2544 | 789.0 | 666.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 17.95 | 21.21 | 1.72 | 353.73 | 0.2628 | 488.0 | 318.5 | |
| 5.72 | 7.08 | 2.93 | 3.62 | 17.26 | 20.79 | 1.30 | 355.02 | 0.2504 | 1068.2 | 786.8 | |
| 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. | |