| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.74 | 51.74 | 12.85 | 31.24 | -15.80 | 246.07 | -30.96 | 119.77 | 0.5708 | 209.0 | -102.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.26 | 3.71 | 1.89 | 2.16 | -15.40 | 249.71 | -27.31 | 121.85 | 0.5228 | 958.6 | 763.6 | |
| 0.00 | 2.45 | 0.00 | 1.43 | -15.78 | 249.33 | -27.69 | 122.16 | 0.5302 | 437.0 | 399.2 | |
| 5.44 | 18.30 | 3.17 | 10.66 | -15.50 | 249.34 | -27.68 | 121.69 | 0.5282 | 895.1 | 770.8 | |
| 8.15 | -3.00 | 4.75 | -3.00 | -15.18 | 249.21 | -27.81 | 121.05 | 0.5277 | 899.3 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.14 | -16.69 | 247.49 | -29.53 | 122.09 | 0.5594 | 737.0 | 619.3 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -14.75 | 247.65 | -29.37 | 119.07 | 0.5447 | 668.0 | 596.5 | |
| 1.63 | 3.08 | 0.98 | 1.85 | -15.42 | 245.94 | -31.08 | 118.91 | 0.5707 | 735.7 | 755.3 | |
| 0.00 | 1.54 | 0.00 | 0.94 | -14.99 | 244.41 | -32.61 | 117.19 | 0.5874 | 602.0 | 473.6 | |
| 0.00 | 0.82 | 0.00 | 0.51 | -16.10 | 243.68 | -33.34 | 118.44 | 0.6027 | -708.0 | -576.2 | |
| 0.00 | 0.63 | 0.00 | 0.40 | -16.01 | 243.17 | -33.85 | 117.98 | 0.6085 | -883.0 | -821.6 | |
| 0.00 | 1.00 | 0.00 | 0.62 | -15.50 | 243.15 | -33.87 | 117.19 | 0.6060 | -856.0 | -715.5 | |
| 0.00 | 1.45 | 0.00 | 0.90 | -15.92 | 243.03 | -33.99 | 117.75 | 0.6097 | -751.0 | -647.5 | |
| 1.27 | 2.72 | 0.80 | 1.72 | -16.18 | 242.17 | -34.85 | 117.62 | 0.6216 | -706.5 | -530.9 | |
| 1.99 | 8.88 | 1.26 | 5.63 | -16.66 | 242.03 | -34.99 | 118.24 | 0.6258 | -952.3 | -732.3 | |
| 0.00 | 1.36 | 0.00 | 0.85 | -15.67 | 242.24 | -34.79 | 116.89 | 0.6181 | -811.0 | -725.4 | |
| 0.00 | 1.54 | 0.00 | 0.98 | -17.01 | 241.88 | -35.14 | 118.67 | 0.6295 | -761.0 | -604.5 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -16.34 | 241.75 | -35.27 | 117.61 | 0.6275 | -566.0 | -439.7 | |
| 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. | |