| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.03 | 0.00 | 14.10 | -10.56 | 337.77 | -19.07 | 126.10 | 0.4011 | -230.6 | -272.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 0.68 | -9.75 | 343.02 | -13.82 | 133.52 | 0.3262 | 923.0 | 742.7 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -8.39 | 342.67 | -14.17 | 129.60 | 0.3157 | 764.0 | 680.3 | |
| 0.00 | 1.64 | 0.00 | 0.84 | -1.31 | 342.71 | -14.13 | 107.74 | 0.2574 | 718.0 | 488.1 | |
| 0.00 | 2.07 | 0.00 | 1.10 | -10.36 | 340.87 | -15.97 | 130.77 | 0.3590 | 752.0 | 634.6 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -13.26 | 340.24 | -16.60 | 135.42 | 0.3978 | 725.0 | 566.0 | |
| 0.00 | 8.53 | 0.00 | 4.67 | -12.39 | 336.84 | -19.99 | 128.59 | 0.4291 | -927.0 | -662.0 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -10.28 | 336.55 | -20.29 | 124.08 | 0.4136 | -705.0 | -520.0 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -9.85 | 336.58 | -20.26 | 123.23 | 0.4096 | -856.0 | -676.8 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -12.19 | 336.34 | -20.50 | 127.53 | 0.4334 | -740.0 | -506.1 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -10.19 | 336.43 | -20.41 | 123.74 | 0.4145 | -949.0 | -728.4 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -11.19 | 335.65 | -21.19 | 124.72 | 0.4333 | -706.0 | -536.2 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -8.51 | 335.41 | -21.43 | 118.99 | 0.4148 | -685.0 | -537.5 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -10.93 | 334.56 | -22.28 | 122.93 | 0.4454 | -815.0 | -697.5 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -10.77 | 333.82 | -23.02 | 121.78 | 0.4538 | -727.0 | -534.7 | |
| 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. | |