| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.71 | 45.52 | 6.65 | 27.47 | 16.36 | 27.68 | 28.03 | 307.94 | 0.5728 | 63.1 | 156.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.14 | 15.56 | 4.44 | 9.68 | 15.95 | 30.98 | 31.33 | 304.19 | 0.6067 | -948.6 | -468.4 | |
| 3.57 | 5.36 | 2.21 | 3.31 | 16.08 | 30.28 | 30.64 | 304.95 | 0.5996 | -836.5 | -593.5 | |
| 0.00 | 1.19 | 0.00 | 0.73 | 16.06 | 29.82 | 30.17 | 305.32 | 0.5941 | -656.0 | -525.9 | |
| 0.00 | 1.19 | 0.00 | 0.73 | 15.79 | 29.17 | 29.52 | 305.49 | 0.5846 | -849.0 | -757.4 | |
| 0.00 | 0.85 | 0.00 | 0.51 | 15.98 | 27.76 | 28.11 | 307.07 | 0.5699 | 532.0 | 429.2 | |
| 0.00 | 1.79 | 0.00 | 1.06 | 15.78 | 26.66 | 27.01 | 307.85 | 0.5557 | 749.0 | 573.0 | |
| 0.00 | 1.45 | 0.00 | 0.85 | 16.05 | 25.39 | 25.75 | 309.55 | 0.5436 | -788.0 | -696.0 | |
| 0.00 | 1.53 | 0.00 | 0.90 | 16.71 | 25.18 | 25.53 | 310.74 | 0.5470 | 620.0 | 507.1 | |
| 0.00 | 3.57 | 0.00 | 2.11 | 17.29 | 24.69 | 25.04 | 312.12 | 0.5470 | 853.0 | 677.6 | |
| 0.00 | 2.04 | 0.00 | 1.20 | 17.13 | 24.49 | 24.84 | 312.10 | 0.5433 | 876.0 | 757.2 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 17.00 | 24.40 | 24.76 | 312.01 | 0.5412 | 911.0 | 690.8 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 16.20 | 24.26 | 24.61 | 311.02 | 0.5322 | 760.0 | 610.1 | |
| 0.00 | 1.79 | 0.00 | 1.04 | 15.81 | 23.90 | 24.26 | 310.84 | 0.5246 | 624.0 | 642.3 | |
| 0.00 | 0.60 | 0.00 | 0.34 | 16.02 | 23.43 | 23.78 | 311.70 | 0.5212 | 683.0 | 500.7 | |
| 0.00 | 1.70 | 0.00 | 0.98 | 15.85 | 23.14 | 23.49 | 311.79 | 0.5164 | 883.0 | 838.8 | |
| 0.00 | 2.30 | 0.00 | 1.33 | 16.31 | 22.63 | 22.98 | 313.08 | 0.5151 | 917.0 | 764.5 | |
| 0.00 | 1.53 | 0.00 | 0.91 | 20.03 | 23.09 | 23.44 | 317.66 | 0.5572 | 688.0 | 553.3 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 17.79 | 22.55 | 22.91 | 315.31 | 0.5291 | 687.0 | 521.5 | |
| 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. | |