| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.88 | 56.91 | 8.86 | 33.14 | 16.45 | 26.85 | 23.94 | 312.46 | 0.5280 | 83.4 | 242.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.22 | 17.69 | 6.74 | 10.63 | 16.04 | 30.83 | 27.91 | 307.33 | 0.5680 | -880.1 | -397.2 | |
| 0.00 | 1.79 | 0.00 | 1.06 | 15.70 | 30.05 | 27.13 | 307.58 | 0.5562 | -718.0 | -547.6 | |
| 1.36 | 5.27 | 0.81 | 3.14 | 16.14 | 30.01 | 27.10 | 308.27 | 0.5595 | -827.5 | -764.8 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 17.31 | 25.56 | 22.64 | 314.95 | 0.5213 | 848.0 | 707.6 | |
| 0.51 | 2.38 | 0.29 | 1.37 | 16.44 | 25.01 | 22.10 | 314.37 | 0.5067 | -696.5 | -601.2 | |
| 0.00 | 1.53 | 0.00 | 0.88 | 17.23 | 24.78 | 21.86 | 315.80 | 0.5123 | 701.0 | 593.2 | |
| 0.00 | 2.21 | 0.00 | 1.26 | 16.33 | 24.50 | 21.59 | 314.86 | 0.5001 | 719.0 | 605.7 | |
| 1.79 | 6.72 | 1.02 | 3.85 | 16.93 | 24.51 | 21.59 | 315.73 | 0.5064 | 852.4 | 610.1 | |
| 0.00 | 1.53 | 0.00 | 0.87 | 16.23 | 24.26 | 21.34 | 315.03 | 0.4965 | 879.0 | 779.6 | |
| 0.00 | 3.49 | 0.00 | 1.99 | 16.64 | 24.31 | 21.39 | 315.57 | 0.5013 | 715.0 | 695.4 | |
| 0.00 | 1.70 | 0.00 | 0.97 | 16.83 | 24.23 | 21.31 | 315.95 | 0.5024 | 589.0 | 605.6 | |
| 0.00 | 0.51 | 0.00 | 0.29 | 16.10 | 23.88 | 20.96 | 315.33 | 0.4910 | 803.0 | 693.0 | |
| 0.00 | 3.49 | 0.00 | 1.96 | 15.88 | 22.97 | 20.06 | 316.26 | 0.4791 | 453.0 | 651.3 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 20.19 | 23.10 | 20.18 | 321.98 | 0.5279 | 655.0 | 576.6 | |
| 0.00 | 3.40 | 0.00 | 1.91 | 16.15 | 22.51 | 19.60 | 317.32 | 0.4772 | 742.0 | 714.1 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 15.94 | 21.81 | 18.89 | 318.04 | 0.4676 | 769.0 | 650.1 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 18.24 | 21.24 | 18.32 | 322.13 | 0.4883 | 741.0 | 643.9 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 18.53 | 21.17 | 18.25 | 322.60 | 0.4910 | 725.0 | 667.5 | |
| 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. | |