| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.02 | 70.46 | 12.35 | 37.83 | 17.28 | 41.83 | -13.64 | 35.74 | 0.3852 | -216.7 | -105.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.07 | 0.00 | 1.62 | 18.07 | 48.57 | -6.90 | 19.60 | 0.3419 | 937.0 | 675.1 | |
| 0.00 | 1.26 | 0.00 | 0.68 | 19.49 | 44.76 | -10.71 | 26.98 | 0.3878 | 708.0 | 571.4 | |
| 6.77 | 26.38 | 3.61 | 14.08 | 17.79 | 43.82 | -11.64 | 31.31 | 0.3714 | -1087.6 | -322.7 | |
| 8.13 | 10.12 | 4.32 | 5.38 | 17.05 | 43.42 | -12.05 | 33.31 | 0.3650 | -1005.8 | -959.7 | |
| 0.54 | 2.26 | 0.29 | 1.20 | 16.77 | 43.01 | -12.45 | 34.63 | 0.3649 | -977.3 | -731.2 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 15.72 | 41.98 | -13.49 | 38.58 | 0.3616 | -862.0 | -642.8 | |
| 2.62 | 3.88 | 1.40 | 2.07 | 16.13 | 41.56 | -13.91 | 38.68 | 0.3710 | -896.7 | -762.3 | |
| 0.00 | 2.08 | 0.00 | 1.11 | 15.82 | 41.35 | -14.11 | 39.65 | 0.3692 | -892.0 | -804.7 | |
| 0.00 | 2.80 | 0.00 | 1.49 | 16.04 | 41.27 | -14.19 | 39.41 | 0.3728 | -674.0 | -685.9 | |
| 0.00 | 1.26 | 0.00 | 0.68 | 15.38 | 40.11 | -15.35 | 42.80 | 0.3773 | -866.0 | -657.2 | |
| 0.00 | 2.26 | 0.00 | 1.22 | 15.29 | 38.35 | -17.12 | 46.01 | 0.3963 | 837.0 | 533.9 | |
| 3.70 | 5.24 | 2.03 | 2.87 | 17.42 | 37.62 | -17.85 | 43.37 | 0.4277 | 867.8 | 606.2 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 16.82 | 36.91 | -18.56 | 45.48 | 0.4290 | 763.0 | 623.8 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 16.31 | 36.79 | -18.67 | 46.55 | 0.4250 | 722.0 | 584.2 | |
| 0.00 | 2.08 | 0.00 | 1.16 | 19.33 | 36.36 | -19.11 | 42.18 | 0.4620 | 928.0 | 731.1 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 17.27 | 35.14 | -20.33 | 47.22 | 0.4538 | 634.0 | 452.0 | |
| 1.26 | 2.26 | 0.70 | 1.25 | 17.05 | 34.99 | -20.47 | 47.79 | 0.4533 | 865.6 | 843.3 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 17.27 | 34.90 | -20.57 | 47.53 | 0.4566 | 691.0 | 549.1 | |
| 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. | |