| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.08 | 215.87 | 71.32 | 344.29 | -18.42 | 124.07 | -70.16 | 110.08 | 0.9507 | 326.8 | 29.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.85 | 192.13 | 19.36 | 292.78 | -18.78 | 125.25 | -68.98 | 110.62 | 0.9457 | 583.5 | 115.1 | |
| 12.59 | -1.00 | 18.55 | -1.00 | -17.86 | 125.62 | -68.62 | 109.71 | 0.9430 | 761.3 | 999999 | |
| 2.40 | -1.00 | 3.72 | -1.00 | -18.67 | 124.63 | -69.60 | 110.41 | 0.9489 | -120.0 | 999999 | |
| 0.00 | 0.69 | 0.00 | 1.25 | -20.78 | 121.91 | -72.33 | 112.21 | 0.9634 | -366.0 | -337.0 | |
| 8.48 | -1.00 | 13.15 | -1.00 | -18.17 | 124.55 | -69.69 | 109.88 | 0.9489 | 180.3 | 999999 | |
| 6.85 | -1.00 | 10.84 | -1.00 | -17.69 | 124.06 | -70.17 | 109.30 | 0.9510 | 197.1 | 999999 | |
| 0.00 | 2.74 | 0.00 | 5.06 | -19.81 | 121.47 | -72.77 | 111.15 | 0.9647 | -631.0 | -536.8 | |
| 0.77 | 6.17 | 1.47 | 11.70 | -20.05 | 120.96 | -73.28 | 111.33 | 0.9670 | -386.9 | -399.7 | |
| 2.14 | 5.65 | 4.23 | 11.17 | -19.50 | 120.29 | -73.95 | 110.68 | 0.9694 | -10.8 | -77.3 | |
| 0.00 | 0.69 | 0.00 | 1.29 | -18.35 | 120.98 | -73.26 | 109.58 | 0.9659 | -352.0 | -314.9 | |
| 0.00 | 0.77 | 0.00 | 2.08 | -19.83 | 116.08 | -78.16 | 110.55 | 0.9841 | -501.0 | -511.4 | |
| 0.00 | 2.66 | 0.00 | 7.13 | -19.64 | 116.10 | -78.14 | 110.36 | 0.9840 | -487.0 | -448.3 | |
| 0.00 | 2.83 | 0.00 | 7.62 | -19.13 | 116.19 | -78.05 | 109.85 | 0.9836 | -494.0 | -492.4 | |
| 0.00 | 1.54 | 0.00 | 4.21 | -18.85 | 116.03 | -78.20 | 109.56 | 0.9839 | -436.0 | -440.9 | |
| 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. | |