| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.78 | 105.70 | 14.25 | 58.29 | -15.72 | 65.51 | 12.54 | 208.30 | 0.4424 | 541.1 | 408.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.82 | 7.47 | 2.12 | 4.15 | -15.83 | 66.87 | 13.89 | 210.77 | 0.4534 | 873.8 | 566.6 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -16.42 | 66.81 | 13.84 | 209.99 | 0.4608 | 704.0 | 581.2 | |
| 0.00 | 2.04 | 0.00 | 1.13 | -15.63 | 66.69 | 13.72 | 210.69 | 0.4494 | 285.0 | 223.7 | |
| 2.49 | 5.69 | 1.38 | 3.16 | -15.85 | 66.48 | 13.51 | 210.04 | 0.4507 | 887.2 | 481.6 | |
| 0.00 | 1.24 | 0.00 | 0.72 | -20.39 | 66.61 | 13.64 | 205.65 | 0.5125 | 620.0 | 458.2 | |
| 5.60 | 73.17 | 3.10 | 40.32 | -15.68 | 66.18 | 13.21 | 209.69 | 0.4460 | 1007.9 | 515.1 | |
| 0.00 | 2.93 | 0.00 | 1.63 | -16.24 | 66.22 | 13.24 | 209.12 | 0.4538 | 678.0 | 599.0 | |
| 5.78 | -6.00 | 3.19 | -6.00 | -15.58 | 66.05 | 13.07 | 209.55 | 0.4436 | 1098.4 | 999999 | |
| 8.09 | -6.00 | 4.46 | -6.00 | -15.40 | 65.78 | 12.80 | 209.24 | 0.4392 | 1234.9 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.64 | -15.96 | 65.72 | 12.74 | 208.50 | 0.4463 | 680.0 | 493.7 | |
| 0.00 | 1.33 | 0.00 | 0.75 | -18.35 | 63.84 | 10.86 | 202.61 | 0.4672 | 592.0 | 419.9 | |
| 0.00 | 2.93 | 0.00 | 1.56 | -12.44 | 61.13 | 8.15 | 202.44 | 0.3642 | 261.0 | 261.9 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -16.96 | 61.10 | 8.13 | 198.32 | 0.4320 | -566.0 | -512.5 | |
| 0.00 | 0.62 | 0.00 | 0.34 | -18.32 | 58.83 | 5.85 | 192.67 | 0.4430 | -627.0 | -507.1 | |
| 0.00 | 1.51 | 0.00 | 0.82 | -16.69 | 58.71 | 5.74 | 193.31 | 0.4176 | -769.0 | -682.4 | |
| 0.00 | 0.98 | 0.00 | 0.54 | -18.21 | 58.66 | 5.69 | 192.38 | 0.4409 | -776.0 | -632.9 | |
| 0.00 | 1.69 | 0.00 | 0.92 | -16.59 | 58.52 | 5.54 | 192.94 | 0.4153 | -767.0 | -671.4 | |
| 0.00 | 0.80 | 0.00 | 0.43 | -16.48 | 58.23 | 5.26 | 192.34 | 0.4127 | -783.0 | -544.2 | |
| 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. | |