| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.36 | 293.36 | 91.94 | 377.41 | -13.18 | 107.29 | -68.09 | 101.34 | 0.9224 | 79.0 | -174.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.60 | 0.00 | 0.46 | -16.15 | 126.02 | -49.36 | 105.20 | 0.7577 | 518.0 | 447.7 | |
| 0.00 | 1.03 | 0.00 | 0.77 | -11.30 | 126.83 | -48.55 | 98.78 | 0.7460 | 587.0 | 498.8 | |
| 0.00 | 0.52 | 0.00 | 0.38 | -11.49 | 126.60 | -48.78 | 99.03 | 0.7487 | 481.0 | 492.5 | |
| 0.00 | 1.81 | 0.00 | 1.38 | -14.80 | 125.51 | -49.87 | 103.37 | 0.7622 | 530.0 | 451.5 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -11.19 | 126.30 | -49.08 | 98.63 | 0.7520 | 618.0 | 586.0 | |
| 0.00 | 1.21 | 0.00 | 0.94 | -6.06 | 124.57 | -50.81 | 91.96 | 0.7735 | 388.0 | 264.9 | |
| 0.00 | 0.60 | 0.00 | 0.64 | -15.22 | 112.38 | -63.00 | 103.46 | 0.8860 | -365.0 | -321.4 | |
| 0.00 | 0.95 | 0.00 | 1.03 | -12.81 | 111.59 | -63.79 | 100.77 | 0.8924 | -387.0 | -355.7 | |
| 0.00 | 0.69 | 0.00 | 0.76 | -12.76 | 111.34 | -64.04 | 100.71 | 0.8944 | -394.0 | -364.0 | |
| 0.00 | 1.12 | 0.00 | 1.22 | -12.58 | 111.42 | -63.96 | 100.52 | 0.8938 | -261.0 | -255.5 | |
| 0.00 | 2.93 | 0.00 | 3.22 | -12.24 | 111.29 | -64.08 | 100.13 | 0.8948 | 245.0 | 99.9 | |
| 0.00 | 0.86 | 0.00 | 0.99 | -14.41 | 109.82 | -65.56 | 102.60 | 0.9053 | 260.0 | 220.2 | |
| 0.00 | 0.52 | 0.00 | 0.65 | -17.54 | 107.55 | -67.83 | 106.06 | 0.9205 | -264.0 | -219.5 | |
| 26.77 | 277.16 | 34.02 | 360.61 | -13.85 | 107.32 | -68.06 | 102.06 | 0.9226 | -636.6 | -183.0 | |
| 1.81 | -14.00 | 2.38 | -14.00 | -14.58 | 106.43 | -68.95 | 102.87 | 0.9282 | -231.0 | 999999 | |
| 0.00 | 3.10 | 0.00 | 4.17 | -15.16 | 105.92 | -69.46 | 103.52 | 0.9312 | -506.0 | -413.3 | |
| 42.78 | -14.00 | 55.54 | -14.00 | -12.70 | 106.84 | -68.54 | 100.83 | 0.9260 | 524.4 | 999999 | |
| 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. | |