| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.61 | 88.58 | 10.47 | 44.99 | -4.63 | 31.24 | 4.71 | 202.36 | 0.2200 | 412.0 | 405.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.98 | 27.64 | 5.59 | 14.06 | -4.09 | 33.67 | 7.14 | 213.37 | 0.2266 | 1151.9 | 751.7 | |
| 1.08 | 3.96 | 0.55 | 2.01 | -4.13 | 32.01 | 5.49 | 206.75 | 0.2130 | 1017.6 | 878.8 | |
| 0.00 | 3.87 | 0.00 | 1.97 | -4.62 | 32.02 | 5.50 | 205.75 | 0.2207 | 897.0 | 724.6 | |
| 1.35 | 15.49 | 0.68 | 7.85 | -4.40 | 31.71 | 5.19 | 204.91 | 0.2150 | 1205.4 | 954.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -5.02 | 31.32 | 4.79 | 202.13 | 0.2220 | 934.0 | 793.8 | |
| 4.41 | 9.00 | 2.24 | 4.57 | -4.79 | 30.83 | 4.30 | 200.41 | 0.2154 | 1098.2 | 765.6 | |
| 0.00 | 5.31 | 0.00 | 2.70 | -5.32 | 30.77 | 4.25 | 199.34 | 0.2236 | 885.0 | 811.6 | |
| 0.00 | 2.07 | 0.00 | 1.05 | -4.85 | 30.46 | 3.94 | 198.71 | 0.2143 | 707.0 | 542.2 | |
| 0.00 | 5.58 | 0.00 | 2.83 | -5.43 | 29.15 | 2.63 | 192.15 | 0.2179 | -819.0 | -870.6 | |
| 0.00 | 2.16 | 0.00 | 1.10 | -5.77 | 29.06 | 2.54 | 191.43 | 0.2233 | -911.0 | -596.2 | |
| 0.99 | 8.01 | 0.50 | 4.05 | -4.59 | 28.91 | 2.38 | 191.83 | 0.2030 | -1028.2 | -897.1 | |
| 1.80 | -11.00 | 0.91 | -11.00 | -4.34 | 28.78 | 2.26 | 191.49 | 0.1984 | -977.8 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.73 | -5.36 | 23.24 | -3.28 | 164.86 | 0.2195 | -727.0 | -604.2 | |
| 0.00 | 1.35 | 0.00 | 0.70 | -8.52 | 22.66 | -3.86 | 165.85 | 0.2739 | -817.0 | -633.7 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -6.55 | 22.07 | -4.46 | 161.52 | 0.2447 | -1001.0 | -717.6 | |
| 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. | |