| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.60 | 0.00 | 10.74 | 8.43 | 26.35 | -1.27 | 164.54 | 0.0783 | -73.1 | -106.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.61 | 0.00 | 1.30 | 5.80 | 33.32 | 5.70 | 260.08 | 0.1008 | -759.0 | -518.9 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 4.86 | 30.72 | 3.09 | 237.58 | 0.0640 | -883.0 | -703.9 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 6.20 | 30.17 | 2.55 | 256.22 | 0.0458 | -931.0 | -800.8 | |
| 0.00 | 1.44 | 0.00 | 0.71 | 7.38 | 29.14 | 1.52 | 290.44 | 0.0282 | -1018.0 | -761.6 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 7.02 | 29.11 | 1.49 | 277.64 | 0.0261 | -934.0 | -759.0 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 6.32 | 28.68 | 1.06 | 244.61 | 0.0204 | -819.0 | -595.6 | |
| 0.00 | 3.24 | 0.00 | 1.61 | 8.60 | 28.29 | 0.67 | 339.61 | 0.0332 | -881.0 | -853.8 | |
| 0.00 | 1.98 | 0.00 | 0.98 | 10.12 | 27.18 | -0.44 | 7.44 | 0.0583 | -892.0 | -636.1 | |
| 0.00 | 1.53 | 0.00 | 0.76 | 9.09 | 26.23 | -1.39 | 31.21 | 0.0464 | 780.0 | 506.0 | |
| 0.00 | 0.81 | 0.00 | 0.40 | 9.92 | 22.34 | -5.28 | 59.01 | 0.1062 | 913.0 | 728.2 | |
| 0.00 | 1.89 | 0.00 | 0.94 | 9.73 | 22.28 | -5.34 | 60.80 | 0.1055 | 958.0 | 865.7 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 9.76 | 21.94 | -5.68 | 62.03 | 0.1109 | 1070.0 | 845.0 | |
| 0.00 | 2.07 | 0.00 | 1.03 | 8.39 | 21.65 | -5.97 | 74.79 | 0.1071 | 792.0 | 681.0 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 12.57 | 18.19 | -9.43 | 57.56 | 0.1904 | 773.0 | 576.0 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 11.29 | 16.69 | -10.93 | 66.73 | 0.2033 | 735.0 | 550.0 | |
| 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. | |