| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.23 | 79.36 | 25.10 | 60.65 | 7.88 | 134.39 | 47.37 | 286.87 | 0.7634 | 162.3 | 321.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.96 | 16.08 | 10.71 | 13.27 | 7.42 | 138.23 | 51.20 | 284.95 | 0.8022 | -680.5 | -426.2 | |
| 0.00 | 0.61 | 0.00 | 0.49 | 8.10 | 137.29 | 50.27 | 286.08 | 0.7946 | -391.0 | -353.3 | |
| 0.00 | 1.04 | 0.00 | 0.84 | 7.92 | 137.07 | 50.05 | 285.94 | 0.7919 | -485.0 | -479.6 | |
| 2.25 | 4.58 | 1.76 | 3.58 | 8.32 | 135.48 | 48.45 | 286.98 | 0.7766 | 497.2 | 299.9 | |
| 0.00 | 1.12 | 0.00 | 0.86 | 7.79 | 134.76 | 47.73 | 286.59 | 0.7673 | 424.0 | 351.3 | |
| 0.00 | 1.56 | 0.00 | 1.18 | 6.35 | 134.42 | 47.40 | 284.89 | 0.7593 | -597.0 | -448.2 | |
| 0.69 | 2.51 | 0.53 | 1.91 | 7.53 | 134.27 | 47.25 | 286.44 | 0.7613 | 665.1 | 545.1 | |
| 0.00 | 1.12 | 0.00 | 0.85 | 7.22 | 134.23 | 47.20 | 286.06 | 0.7598 | 521.0 | 485.4 | |
| 0.95 | 3.37 | 0.71 | 2.53 | 6.69 | 133.85 | 46.82 | 285.53 | 0.7541 | -725.8 | -519.5 | |
| 0.00 | 1.99 | 0.00 | 1.50 | 7.33 | 133.80 | 46.78 | 286.36 | 0.7556 | 580.0 | 513.0 | |
| 0.00 | 0.86 | 0.00 | 0.66 | 8.90 | 133.87 | 46.85 | 288.32 | 0.7615 | 511.0 | 419.2 | |
| 0.00 | 1.56 | 0.00 | 1.18 | 8.76 | 133.62 | 46.60 | 288.23 | 0.7584 | 680.0 | 543.8 | |
| 0.00 | 0.78 | 0.00 | 0.59 | 8.70 | 133.35 | 46.33 | 288.27 | 0.7553 | 665.0 | 524.9 | |
| 0.00 | 1.47 | 0.00 | 1.10 | 8.94 | 133.22 | 46.19 | 288.62 | 0.7546 | 499.0 | 425.5 | |
| 0.00 | 0.95 | 0.00 | 0.71 | 7.68 | 132.94 | 45.91 | 287.13 | 0.7472 | 620.0 | 504.8 | |
| 0.00 | 0.69 | 0.00 | 0.51 | 6.96 | 132.79 | 45.77 | 286.26 | 0.7432 | 481.0 | 433.9 | |
| 5.53 | 39.07 | 4.10 | 28.89 | 7.94 | 132.76 | 45.73 | 287.53 | 0.7461 | 719.6 | 543.8 | |
| 9.85 | -17.00 | 7.29 | -17.00 | 8.32 | 132.55 | 45.53 | 288.10 | 0.7452 | 842.1 | 999999 | |
| 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. | |