| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.41 | 56.21 | 11.01 | 28.94 | 17.92 | 325.22 | -9.45 | 35.22 | 0.2702 | 382.4 | 176.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.09 | 0.00 | 1.06 | 17.37 | 329.88 | -4.79 | 20.95 | 0.2239 | 790.0 | 558.5 | |
| 7.57 | 15.92 | 3.86 | 8.13 | 17.00 | 326.82 | -7.85 | 32.85 | 0.2420 | -1100.2 | -813.0 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 17.46 | 326.70 | -7.97 | 32.18 | 0.2495 | -780.0 | -555.5 | |
| 3.22 | 6.61 | 1.65 | 3.38 | 17.21 | 326.40 | -8.27 | 33.71 | 0.2488 | -906.8 | -714.3 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 18.11 | 325.34 | -9.33 | 34.81 | 0.2712 | 991.0 | 776.9 | |
| 0.00 | 2.61 | 0.00 | 1.34 | 17.44 | 325.03 | -9.64 | 37.25 | 0.2653 | 895.0 | 688.6 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 14.40 | 325.05 | -9.62 | 45.67 | 0.2274 | 934.0 | 734.1 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 18.62 | 324.67 | -10.00 | 35.52 | 0.2845 | 851.0 | 628.5 | |
| 0.00 | 1.13 | 0.00 | 0.59 | 19.26 | 324.51 | -10.17 | 34.61 | 0.2947 | 693.0 | 511.9 | |
| 2.18 | 8.09 | 1.13 | 4.19 | 18.77 | 324.06 | -10.62 | 36.80 | 0.2925 | 1015.2 | 748.4 | |
| 8.44 | 10.44 | 4.37 | 5.40 | 18.43 | 324.01 | -10.66 | 37.65 | 0.2885 | 1162.1 | 893.6 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 18.48 | 323.56 | -11.11 | 38.66 | 0.2939 | 792.0 | 730.4 | |
| 0.00 | 0.78 | 0.00 | 0.41 | 19.14 | 322.68 | -11.99 | 39.29 | 0.3114 | 741.0 | 734.2 | |
| 0.00 | 0.78 | 0.00 | 0.42 | 21.89 | 320.77 | -13.90 | 37.85 | 0.3648 | 746.0 | 624.2 | |
| 0.00 | 1.57 | 0.00 | 0.83 | 20.16 | 319.73 | -14.95 | 43.16 | 0.3555 | 927.0 | 775.7 | |
| 0.00 | 0.52 | 0.00 | 0.28 | 23.02 | 318.54 | -16.13 | 39.83 | 0.4009 | 736.0 | 629.7 | |
| 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. | |