| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.52 | 393.46 | 35.23 | 218.19 | 17.76 | 166.55 | 14.14 | 328.83 | 0.4510 | -596.2 | -310.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.50 | 358.27 | 33.59 | 198.98 | 17.74 | 166.96 | 14.55 | 328.02 | 0.4537 | -1274.6 | -411.9 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 17.22 | 165.42 | 13.01 | 330.19 | 0.4344 | -638.0 | -575.8 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 17.12 | 165.09 | 12.68 | 330.70 | 0.4304 | 446.0 | 294.2 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 17.36 | 163.72 | 11.31 | 333.66 | 0.4236 | 768.0 | 516.0 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 18.00 | 163.27 | 10.87 | 335.23 | 0.4297 | 802.0 | 656.2 | |
| 0.00 | 2.49 | 0.00 | 1.37 | 18.92 | 163.07 | 10.67 | 336.53 | 0.4415 | 685.0 | 533.3 | |
| 0.00 | 2.67 | 0.00 | 1.46 | 18.29 | 163.00 | 10.59 | 336.07 | 0.4321 | 771.0 | 615.2 | |
| 0.00 | 7.11 | 0.00 | 3.89 | 18.03 | 162.86 | 10.45 | 336.10 | 0.4274 | 956.0 | 857.3 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 18.91 | 162.72 | 10.31 | 337.23 | 0.4392 | 605.0 | 520.4 | |
| 0.00 | 0.80 | 0.00 | 0.44 | 17.96 | 162.50 | 10.09 | 336.76 | 0.4241 | 871.0 | 779.3 | |
| 0.00 | 1.87 | 0.00 | 1.03 | 18.91 | 162.52 | 10.12 | 337.61 | 0.4380 | 800.0 | 616.1 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 17.89 | 162.27 | 9.86 | 337.16 | 0.4217 | 668.0 | 608.4 | |
| 0.00 | 0.80 | 0.00 | 0.44 | 18.94 | 162.23 | 9.83 | 338.21 | 0.4367 | 696.0 | 537.2 | |
| 0.00 | 1.24 | 0.00 | 0.68 | 18.51 | 161.85 | 9.45 | 338.59 | 0.4282 | 752.0 | 562.0 | |
| 0.00 | 1.51 | 0.00 | 0.82 | 17.16 | 161.59 | 9.18 | 337.90 | 0.4069 | 834.0 | 710.6 | |
| 0.71 | 3.46 | 0.39 | 1.88 | 17.55 | 161.38 | 8.98 | 338.71 | 0.4114 | 844.0 | 720.0 | |
| 0.71 | 2.49 | 0.39 | 1.35 | 17.64 | 160.40 | 7.99 | 340.94 | 0.4073 | 859.0 | 680.0 | |
| 1.60 | 4.26 | 0.86 | 2.30 | 17.24 | 160.32 | 7.91 | 340.79 | 0.4010 | 1030.1 | 809.1 | |
| 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. | |