| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.79 | 0.00 | 15.06 | 6.61 | 265.30 | -16.28 | 75.50 | 0.2870 | 345.2 | 314.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.50 | 7.17 | 279.89 | -1.68 | 22.64 | 0.0760 | -936.0 | -762.9 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 3.63 | 279.68 | -1.89 | 76.14 | 0.0340 | -830.0 | -515.1 | |
| 0.00 | 2.54 | 0.00 | 1.26 | 3.54 | 278.89 | -2.68 | 82.03 | 0.0474 | -928.0 | -792.5 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 3.22 | 275.46 | -6.11 | 89.30 | 0.1068 | -826.0 | -676.5 | |
| 0.00 | 1.54 | 0.00 | 0.77 | 3.89 | 275.40 | -6.18 | 83.10 | 0.1086 | -760.0 | -617.4 | |
| 0.00 | 3.27 | 0.00 | 1.67 | 9.41 | 269.51 | -12.06 | 61.94 | 0.2346 | 967.0 | 811.2 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 8.40 | 265.09 | -16.48 | 71.57 | 0.2971 | 888.0 | 654.6 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 8.90 | 261.63 | -19.94 | 72.98 | 0.3539 | 860.0 | 701.6 | |
| 0.00 | 3.00 | 0.00 | 1.59 | 8.83 | 261.34 | -20.24 | 73.37 | 0.3582 | 949.0 | 739.0 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 8.83 | 261.11 | -20.47 | 73.54 | 0.3618 | 772.0 | 604.5 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 9.01 | 260.77 | -20.81 | 73.29 | 0.3679 | 868.0 | 701.5 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 9.16 | 260.66 | -20.91 | 72.97 | 0.3702 | 782.0 | 567.2 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 1.51 | 259.51 | -22.06 | 93.80 | 0.3779 | 759.0 | 630.9 | |
| 0.00 | 2.00 | 0.00 | 1.07 | 6.81 | 259.23 | -22.34 | 79.85 | 0.3851 | 774.0 | 616.5 | |
| 0.00 | 1.82 | 0.00 | 0.98 | 7.76 | 258.24 | -23.33 | 77.83 | 0.4031 | 837.0 | 721.3 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 7.57 | 257.82 | -23.75 | 78.47 | 0.4092 | 713.0 | 491.3 | |
| 0.00 | 0.82 | 0.00 | 0.45 | 5.08 | 255.71 | -25.86 | 84.88 | 0.4380 | 766.0 | 582.8 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 4.55 | 249.36 | -32.21 | 86.48 | 0.5345 | 559.0 | 494.8 | |
| 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. | |