| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.18 | 52.72 | 9.85 | 27.05 | 17.74 | 329.01 | -10.51 | 42.70 | 0.2574 | -0.8 | 47.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.49 | 13.66 | 334.36 | -5.16 | 37.37 | 0.1448 | -949.0 | -772.5 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 18.53 | 333.62 | -5.90 | 26.15 | 0.2222 | -870.0 | -642.9 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 18.02 | 332.42 | -7.10 | 31.74 | 0.2245 | -968.0 | -734.6 | |
| 0.00 | 4.84 | 0.00 | 2.47 | 18.23 | 331.83 | -7.69 | 33.26 | 0.2328 | -989.0 | -764.3 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 17.39 | 331.84 | -7.68 | 35.41 | 0.2212 | -996.0 | -744.1 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 18.34 | 331.22 | -8.31 | 34.99 | 0.2402 | -740.0 | -578.1 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 17.97 | 331.20 | -8.32 | 35.99 | 0.2353 | -1016.0 | -798.6 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 17.44 | 331.16 | -8.36 | 37.53 | 0.2287 | -820.0 | -710.9 | |
| 7.26 | 9.24 | 3.74 | 4.76 | 19.13 | 328.77 | -10.75 | 39.98 | 0.2755 | -1017.0 | -773.7 | |
| 1.43 | 2.60 | 0.74 | 1.34 | 18.16 | 328.67 | -10.85 | 42.71 | 0.2649 | 924.6 | 839.0 | |
| 4.84 | 19.82 | 2.48 | 10.15 | 17.14 | 328.54 | -10.98 | 45.91 | 0.2546 | 1144.2 | 778.8 | |
| 5.65 | -11.00 | 2.89 | -11.00 | 16.89 | 328.26 | -11.26 | 47.34 | 0.2551 | 1030.7 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.92 | 16.86 | 326.91 | -12.61 | 50.52 | 0.2720 | 601.0 | 478.6 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 16.34 | 326.91 | -12.61 | 52.09 | 0.2667 | 849.0 | 607.4 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 16.96 | 326.09 | -13.43 | 51.90 | 0.2836 | 813.0 | 566.2 | |
| 0.00 | 1.43 | 0.00 | 0.74 | 14.75 | 326.14 | -13.38 | 58.67 | 0.2631 | 976.0 | 645.9 | |
| 0.00 | 2.06 | 0.00 | 1.07 | 16.82 | 325.42 | -14.11 | 53.58 | 0.2912 | 834.0 | 666.7 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 26.83 | 323.06 | -16.46 | 36.50 | 0.4270 | 558.0 | 450.0 | |
| 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. | |