| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.59 | 0.00 | 13.12 | 13.82 | 60.29 | -11.21 | 140.78 | 0.2447 | -218.6 | -143.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.31 | 0.00 | 0.66 | 14.98 | 73.72 | 2.23 | 346.12 | 0.1571 | -678.0 | -516.7 | |
| 0.00 | 1.67 | 0.00 | 0.84 | 14.16 | 67.13 | -4.36 | 28.15 | 0.1571 | -1030.0 | -807.5 | |
| 0.00 | 1.23 | 0.00 | 0.62 | 14.24 | 66.85 | -4.64 | 29.37 | 0.1607 | -892.0 | -722.1 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 12.88 | 66.44 | -5.05 | 36.50 | 0.1449 | -887.0 | -719.3 | |
| 0.00 | 1.23 | 0.00 | 0.61 | 13.06 | 66.13 | -5.36 | 37.39 | 0.1506 | -772.0 | -505.2 | |
| 0.00 | 1.49 | 0.00 | 0.75 | 12.30 | 65.07 | -6.42 | 45.87 | 0.1530 | -951.0 | -667.6 | |
| 0.00 | 1.84 | 0.00 | 0.93 | 14.78 | 63.13 | -8.36 | 43.26 | 0.2061 | -1008.0 | -824.6 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 10.82 | 62.64 | -8.85 | 61.80 | 0.1723 | -959.0 | -780.5 | |
| 0.00 | 1.75 | 0.00 | 0.89 | 13.98 | 62.26 | -9.24 | 48.90 | 0.2076 | -921.0 | -728.7 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 18.47 | 59.93 | -11.57 | 41.66 | 0.2874 | -680.0 | -487.2 | |
| 0.00 | 1.31 | 0.00 | 0.67 | 13.18 | 59.66 | -11.83 | 58.39 | 0.2355 | 720.0 | 611.3 | |
| 0.00 | 1.67 | 0.00 | 0.87 | 19.62 | 59.17 | -12.33 | 40.72 | 0.3097 | -826.0 | -625.5 | |
| 0.00 | 1.14 | 0.00 | 0.58 | 13.75 | 58.18 | -13.31 | 59.20 | 0.2616 | 882.0 | 741.8 | |
| 0.00 | 1.84 | 0.00 | 0.96 | 12.09 | 53.75 | -17.74 | 70.28 | 0.3179 | 919.0 | 725.7 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 12.02 | 53.57 | -17.93 | 70.64 | 0.3205 | 825.0 | 531.6 | |
| 0.00 | 2.37 | 0.00 | 1.25 | 12.04 | 52.34 | -19.16 | 71.59 | 0.3397 | 799.0 | 637.1 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 12.20 | 51.77 | -19.72 | 71.56 | 0.3492 | 642.0 | 554.9 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 14.43 | 49.87 | -21.63 | 67.24 | 0.3888 | 883.0 | 612.6 | |
| 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. | |