| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.21 | 56.68 | 9.31 | 28.90 | 15.02 | 243.66 | 8.43 | 322.82 | 0.2358 | -146.6 | 145.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.70 | 22.37 | 7.02 | 11.47 | 14.39 | 246.67 | 11.45 | 311.58 | 0.2581 | -1094.9 | -605.0 | |
| 0.00 | 3.81 | 0.00 | 1.94 | 14.11 | 245.25 | 10.02 | 314.41 | 0.2374 | -836.0 | -698.0 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 15.03 | 244.23 | 9.00 | 320.12 | 0.2368 | -1097.0 | -902.5 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 12.98 | 243.87 | 8.65 | 314.83 | 0.2075 | 703.0 | 448.3 | |
| 4.51 | 6.42 | 2.29 | 3.26 | 14.37 | 243.68 | 8.45 | 319.98 | 0.2223 | -1043.8 | -847.5 | |
| 0.00 | 1.56 | 0.00 | 0.79 | 15.59 | 242.63 | 7.41 | 326.88 | 0.2282 | 821.0 | 643.9 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 16.85 | 242.12 | 6.89 | 331.52 | 0.2418 | 869.0 | 573.9 | |
| 0.00 | 1.21 | 0.00 | 0.61 | 14.82 | 240.59 | 5.36 | 332.92 | 0.1995 | 833.0 | 677.6 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 16.49 | 240.51 | 5.28 | 336.73 | 0.2246 | 882.0 | 756.5 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 14.83 | 240.31 | 5.09 | 334.14 | 0.1974 | 977.0 | 757.3 | |
| 0.00 | 2.25 | 0.00 | 1.14 | 16.47 | 240.01 | 4.78 | 338.67 | 0.2209 | 1015.0 | 728.6 | |
| 0.00 | 10.14 | 0.00 | 5.15 | 16.47 | 239.55 | 4.32 | 340.59 | 0.2182 | 914.0 | 795.9 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 16.23 | 239.29 | 4.06 | 341.27 | 0.2129 | 937.0 | 721.1 | |
| 0.00 | 1.04 | 0.00 | 0.52 | 14.89 | 239.14 | 3.91 | 339.65 | 0.1905 | 934.0 | 798.7 | |
| 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. | |