| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.55 | 46.69 | 7.17 | 27.43 | 5.64 | 69.84 | -32.48 | 85.94 | 0.5369 | -68.9 | 54.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.51 | 23.95 | 1.42 | 13.59 | 5.61 | 73.20 | -29.12 | 85.88 | 0.4876 | -1101.0 | -757.7 | |
| 2.25 | -1.00 | 1.27 | -1.00 | 5.79 | 73.16 | -29.16 | 85.52 | 0.4883 | -1152.7 | 999999 | |
| 3.29 | -1.00 | 1.87 | -1.00 | 5.88 | 73.01 | -29.31 | 85.35 | 0.4905 | -925.7 | 999999 | |
| 3.29 | -1.00 | 1.87 | -1.00 | 5.60 | 72.86 | -29.46 | 85.92 | 0.4928 | -800.6 | 999999 | |
| 0.00 | 2.42 | 0.00 | 1.38 | 5.28 | 72.87 | -29.45 | 86.59 | 0.4924 | -690.0 | -591.7 | |
| 0.00 | 0.35 | 0.00 | 0.20 | 4.95 | 71.23 | -31.09 | 87.27 | 0.5171 | -408.0 | -469.5 | |
| 0.00 | 1.73 | 0.00 | 1.04 | 6.47 | 67.35 | -34.97 | 84.61 | 0.5743 | 652.0 | 596.7 | |
| 0.00 | 1.82 | 0.00 | 1.10 | 6.01 | 67.01 | -35.31 | 85.43 | 0.5788 | 744.0 | 592.0 | |
| 0.00 | 1.47 | 0.00 | 0.89 | 6.18 | 66.82 | -35.50 | 85.15 | 0.5817 | 790.0 | 583.2 | |
| 0.00 | 0.43 | 0.00 | 0.26 | 6.11 | 66.49 | -35.83 | 85.29 | 0.5862 | 419.0 | 491.8 | |
| 1.21 | 6.48 | 0.74 | 3.98 | 5.46 | 65.91 | -36.41 | 86.41 | 0.5943 | 869.1 | 746.8 | |
| 0.00 | 1.47 | 0.00 | 0.90 | 4.41 | 65.82 | -36.50 | 88.17 | 0.5955 | 641.0 | 486.6 | |
| 0.00 | 2.33 | 0.00 | 1.44 | 5.09 | 65.75 | -36.57 | 87.02 | 0.5966 | 751.0 | 643.2 | |
| 0.00 | 2.16 | 0.00 | 1.35 | 5.65 | 64.73 | -37.59 | 86.11 | 0.6107 | 894.0 | 733.1 | |
| 0.00 | 2.08 | 0.00 | 1.30 | 5.82 | 64.72 | -37.60 | 85.82 | 0.6109 | 637.0 | 570.6 | |
| 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. | |