| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.77 | 145.41 | 22.67 | 98.41 | 6.57 | 203.33 | -42.97 | 84.06 | 0.6829 | -539.8 | -276.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.73 | 0.00 | 0.46 | 6.23 | 207.73 | -38.58 | 84.32 | 0.6252 | -647.0 | -508.0 | |
| 0.00 | 0.82 | 0.00 | 0.54 | 9.23 | 205.05 | -41.25 | 79.94 | 0.6632 | -553.0 | -434.1 | |
| 8.26 | 12.08 | 5.48 | 8.00 | 6.91 | 204.68 | -41.62 | 83.47 | 0.6660 | -901.0 | -623.2 | |
| 0.00 | 2.00 | 0.00 | 1.34 | 7.09 | 203.71 | -42.60 | 83.27 | 0.6786 | -350.0 | -309.1 | |
| 20.34 | 107.62 | 13.67 | 72.33 | 6.36 | 203.74 | -42.56 | 84.35 | 0.6778 | -1025.8 | -339.3 | |
| 0.00 | 1.63 | 0.00 | 1.11 | 8.57 | 203.06 | -43.25 | 81.16 | 0.6879 | -585.0 | -466.4 | |
| 2.63 | 10.35 | 1.79 | 7.05 | 7.25 | 203.10 | -43.20 | 83.08 | 0.6864 | -743.7 | -409.8 | |
| 2.54 | -7.00 | 1.73 | -7.00 | 7.15 | 202.82 | -43.49 | 83.24 | 0.6899 | -485.7 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.64 | 3.55 | 200.81 | -45.49 | 88.41 | 0.7143 | -605.0 | -519.0 | |
| 0.00 | 1.18 | 0.00 | 0.85 | 5.85 | 199.56 | -46.75 | 85.21 | 0.7294 | 518.0 | 581.4 | |
| 0.00 | 0.82 | 0.00 | 0.59 | 5.78 | 199.38 | -46.92 | 85.31 | 0.7314 | 642.0 | 570.6 | |
| 0.00 | 0.54 | 0.00 | 0.40 | 5.93 | 199.32 | -46.98 | 85.10 | 0.7322 | 613.0 | 564.2 | |
| 0.00 | 0.91 | 0.00 | 0.69 | 9.82 | 196.96 | -49.34 | 80.02 | 0.7612 | 319.0 | 329.3 | |
| 0.00 | 2.00 | 0.00 | 1.51 | 7.52 | 197.23 | -49.08 | 83.03 | 0.7570 | 716.0 | 622.4 | |
| 0.00 | 0.91 | 0.00 | 0.69 | 7.74 | 197.19 | -49.11 | 82.74 | 0.7574 | 601.0 | 536.8 | |
| 0.00 | 2.00 | 0.00 | 1.52 | 8.24 | 196.78 | -49.53 | 82.10 | 0.7623 | 632.0 | 517.5 | |
| 0.00 | 0.91 | 0.00 | 0.69 | 6.95 | 196.79 | -49.52 | 83.80 | 0.7617 | 577.0 | 488.6 | |
| 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. | |