| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.84 | 0.00 | 10.39 | -19.31 | 73.41 | -37.12 | 126.12 | 0.7015 | 128.1 | 146.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.76 | 0.00 | 1.12 | -18.20 | 79.67 | -30.85 | 129.51 | 0.6337 | 805.0 | 552.5 | |
| 0.00 | 1.40 | 0.00 | 0.88 | -15.42 | 79.96 | -30.56 | 126.09 | 0.6088 | 756.0 | 573.8 | |
| 0.00 | 1.32 | 0.00 | 0.85 | -16.84 | 77.38 | -33.14 | 125.82 | 0.6476 | 835.0 | 737.3 | |
| 0.00 | 0.61 | 0.00 | 0.40 | -17.12 | 76.61 | -33.91 | 125.57 | 0.6578 | 534.0 | 452.4 | |
| 0.00 | 2.11 | 0.00 | 1.38 | -16.90 | 76.55 | -33.98 | 125.23 | 0.6570 | 710.0 | 504.8 | |
| 0.00 | 0.53 | 0.00 | 0.35 | -16.82 | 75.76 | -34.76 | 124.53 | 0.6648 | 551.0 | 379.3 | |
| 0.00 | 0.97 | 0.00 | 0.64 | -16.75 | 75.28 | -35.24 | 124.09 | 0.6696 | 379.0 | 403.1 | |
| 0.00 | 0.97 | 0.00 | 0.70 | -20.58 | 71.83 | -38.69 | 126.38 | 0.7292 | -597.0 | -428.2 | |
| 0.00 | 1.40 | 0.00 | 1.02 | -20.56 | 71.59 | -38.94 | 126.20 | 0.7315 | -298.0 | -277.0 | |
| 0.00 | 1.40 | 0.00 | 1.05 | -21.36 | 69.95 | -40.57 | 126.06 | 0.7516 | -191.0 | -147.6 | |
| 0.00 | 0.44 | 0.00 | 0.36 | -24.80 | 67.40 | -43.13 | 128.35 | 0.7936 | -290.0 | -307.0 | |
| 0.00 | 0.79 | 0.00 | 0.61 | -20.76 | 67.79 | -42.74 | 124.06 | 0.7683 | -522.0 | -480.1 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -20.59 | 67.80 | -42.72 | 123.88 | 0.7673 | -620.0 | -486.0 | |
| 0.00 | 0.88 | 0.00 | 0.83 | -26.55 | 60.78 | -49.75 | 126.70 | 0.8536 | -258.0 | -322.3 | |
| 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. | |