| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.84 | 51.23 | 7.82 | 28.66 | 16.40 | 27.78 | 18.26 | 319.81 | 0.4666 | -39.6 | 54.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.60 | 17.17 | 5.45 | 9.74 | 16.22 | 30.31 | 20.79 | 315.67 | 0.4896 | -996.2 | -672.2 | |
| 0.00 | 3.82 | 0.00 | 2.16 | 16.08 | 29.77 | 20.25 | 316.20 | 0.4824 | -918.0 | -764.4 | |
| 0.59 | 1.78 | 0.33 | 1.00 | 15.88 | 29.35 | 19.83 | 316.48 | 0.4759 | -999.0 | -853.8 | |
| 1.95 | 3.23 | 1.10 | 1.81 | 15.90 | 29.00 | 19.48 | 317.02 | 0.4724 | -1048.3 | -842.5 | |
| 0.00 | 1.53 | 0.00 | 0.86 | 16.72 | 28.98 | 19.47 | 318.25 | 0.4813 | -740.0 | -610.9 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 16.15 | 28.70 | 19.18 | 317.82 | 0.4719 | -765.0 | -621.6 | |
| 0.00 | 1.10 | 0.00 | 0.61 | 15.49 | 27.69 | 18.17 | 318.35 | 0.4542 | 511.0 | 367.8 | |
| 0.85 | 8.16 | 0.47 | 4.53 | 17.31 | 25.74 | 16.22 | 324.10 | 0.4567 | 819.5 | 737.3 | |
| 0.00 | 1.70 | 0.00 | 0.94 | 15.95 | 25.62 | 16.10 | 322.40 | 0.4389 | 786.0 | 516.8 | |
| 0.00 | 0.51 | 0.00 | 0.28 | 17.23 | 24.86 | 15.34 | 325.47 | 0.4478 | 581.0 | 440.5 | |
| 0.85 | 2.04 | 0.47 | 1.13 | 17.03 | 24.75 | 15.23 | 325.41 | 0.4444 | 996.5 | 810.5 | |
| 0.00 | 2.55 | 0.00 | 1.40 | 16.34 | 24.69 | 15.17 | 324.56 | 0.4351 | 682.0 | 652.5 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 17.25 | 24.64 | 15.12 | 325.89 | 0.4462 | 731.0 | 606.9 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 16.20 | 24.24 | 14.72 | 325.19 | 0.4292 | 878.0 | 779.2 | |
| 0.00 | 1.61 | 0.00 | 0.88 | 16.23 | 23.95 | 14.43 | 325.74 | 0.4270 | 768.0 | 622.2 | |
| 0.00 | 1.70 | 0.00 | 0.92 | 15.89 | 22.70 | 13.18 | 327.66 | 0.4116 | 987.0 | 860.2 | |
| 0.00 | 0.68 | 0.00 | 0.37 | 16.23 | 22.28 | 12.76 | 328.93 | 0.4127 | 837.0 | 679.6 | |
| 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. | |