| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.54 | 224.43 | 47.02 | 222.92 | -19.59 | 107.32 | -54.60 | 117.59 | 0.8685 | 555.6 | 224.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.95 | 0.00 | 2.72 | -20.76 | 110.75 | -51.18 | 120.29 | 0.8457 | 21.0 | 69.6 | |
| 0.00 | 0.89 | 0.00 | 0.88 | -23.16 | 109.02 | -52.91 | 122.09 | 0.8677 | -535.0 | -381.5 | |
| 0.00 | 0.71 | 0.00 | 0.71 | -22.40 | 108.40 | -53.52 | 121.03 | 0.8696 | 473.0 | 427.8 | |
| 0.00 | 5.36 | 0.00 | 5.45 | -22.34 | 107.65 | -54.27 | 120.66 | 0.8748 | 561.0 | 398.2 | |
| 0.00 | 1.07 | 0.00 | 1.09 | -22.05 | 107.54 | -54.39 | 120.30 | 0.8747 | 552.0 | 497.2 | |
| 0.00 | 1.52 | 0.00 | 1.48 | -19.87 | 108.10 | -53.83 | 118.19 | 0.8634 | 392.0 | 374.8 | |
| 0.00 | 2.32 | 0.00 | 2.27 | -19.71 | 108.01 | -53.91 | 117.99 | 0.8636 | 654.0 | 530.2 | |
| 5.54 | 131.97 | 5.58 | 132.97 | -20.53 | 107.20 | -54.73 | 118.55 | 0.8724 | 583.1 | 123.4 | |
| 19.30 | 72.64 | 18.66 | 69.87 | -18.69 | 107.96 | -53.97 | 116.86 | 0.8607 | 759.1 | 442.2 | |
| 8.49 | -8.00 | 8.55 | -8.00 | -20.15 | 107.01 | -54.92 | 118.07 | 0.8726 | 632.5 | 999999 | |
| 8.76 | -8.00 | 8.80 | -8.00 | -19.82 | 106.95 | -54.97 | 117.70 | 0.8720 | 604.9 | 999999 | |
| 5.45 | -8.00 | 5.43 | -8.00 | -19.09 | 106.99 | -54.93 | 116.92 | 0.8695 | 569.4 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.76 | -19.67 | 104.65 | -57.27 | 116.68 | 0.8884 | 459.0 | 410.9 | |
| 0.00 | 1.25 | 0.00 | 1.35 | -18.76 | 103.96 | -57.96 | 115.46 | 0.8909 | 480.0 | 406.6 | |
| 0.00 | 0.80 | 0.00 | 0.89 | -18.21 | 103.22 | -58.71 | 114.63 | 0.8948 | -417.0 | -356.4 | |
| 0.00 | 1.97 | 0.00 | 2.18 | -17.82 | 102.87 | -59.05 | 114.10 | 0.8963 | -636.0 | -487.2 | |
| 0.00 | 0.27 | 0.00 | 0.30 | -17.55 | 102.71 | -59.21 | 113.76 | 0.8968 | -456.0 | -464.7 | |
| 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. | |