| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 112 | 673 | 60 | 364 | 2.64 | 271.60 | -23.41 | 93.18 | 0.3991 | 1615.3 | 644.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33 | 615 | 18 | 331 | 2.28 | 272.87 | -22.14 | 94.38 | 0.3794 | 2110.2 | 687.8 | |
| 17 | -1 | 9 | -1 | 2.11 | 272.37 | -22.64 | 94.69 | 0.3877 | 1449.6 | 999999 | |
| 0 | 4 | 0 | 2 | 1.14 | 272.00 | -23.00 | 97.05 | 0.3954 | 657.0 | 596.9 | |
| 13 | -1 | 7 | -1 | 3.41 | 271.92 | -23.08 | 91.27 | 0.3932 | 1611.6 | 999999 | |
| 6 | -1 | 3 | -1 | 2.32 | 271.61 | -23.40 | 93.97 | 0.3995 | 1285.2 | 999999 | |
| 32 | -1 | 17 | -1 | 2.93 | 271.47 | -23.53 | 92.41 | 0.4009 | 1598.0 | 999999 | |
| 8 | -1 | 4 | -1 | 2.92 | 271.14 | -23.87 | 92.38 | 0.4063 | 1167.3 | 999999 | |
| 3 | 9 | 2 | 5 | 4.63 | 270.15 | -24.86 | 88.16 | 0.4210 | 714.3 | 575.7 | |
| 0 | 7 | 0 | 4 | 4.82 | 268.95 | -26.06 | 87.71 | 0.4400 | -625.0 | -629.0 | |
| 0 | 4 | 0 | 2 | 4.08 | 268.85 | -26.16 | 89.38 | 0.4417 | -483.0 | -341.4 | |
| 0 | 6 | 0 | 3 | 4.06 | 268.20 | -26.81 | 89.40 | 0.4518 | 561.0 | 431.1 | |
| 0 | 6 | 0 | 3 | 0.61 | 266.44 | -28.57 | 96.49 | 0.4833 | 890.0 | 768.7 | |
| 0 | 4 | 0 | 3 | 0.63 | 265.82 | -29.18 | 96.29 | 0.4926 | 522.0 | 454.9 | |
| 0 | 8 | 0 | 4 | 2.08 | 265.41 | -29.60 | 93.27 | 0.4965 | 472.0 | 336.5 | |
| 0 | 4 | 0 | 3 | 1.50 | 263.49 | -31.52 | 94.04 | 0.5260 | 471.0 | 577.2 | |
| 0 | 6 | 0 | 4 | 2.76 | 260.18 | -34.82 | 91.28 | 0.5728 | -492.0 | -465.1 | |
| 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. | |