| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.36 | 365.14 | 33.20 | 231.05 | 17.90 | 166.30 | 31.49 | 306.99 | 0.6245 | -744.9 | -305.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.36 | 345.31 | 33.20 | 218.87 | 17.88 | 166.47 | 31.66 | 306.81 | 0.6262 | -1260.8 | -355.9 | |
| 0.00 | 2.22 | 0.00 | 1.38 | 17.35 | 164.86 | 30.04 | 307.48 | 0.6044 | -174.0 | -190.2 | |
| 0.00 | 1.87 | 0.00 | 1.15 | 17.20 | 164.39 | 29.58 | 307.69 | 0.5981 | 591.0 | 501.3 | |
| 0.00 | 1.42 | 0.00 | 0.87 | 17.71 | 163.39 | 28.58 | 309.32 | 0.5913 | 598.0 | 503.6 | |
| 0.00 | 1.60 | 0.00 | 0.98 | 18.07 | 163.35 | 28.54 | 309.85 | 0.5938 | 509.0 | 402.3 | |
| 0.00 | 1.78 | 0.00 | 1.09 | 17.87 | 163.17 | 28.36 | 309.75 | 0.5902 | 786.0 | 708.3 | |
| 0.00 | 1.60 | 0.00 | 0.98 | 18.41 | 162.91 | 28.09 | 310.75 | 0.5920 | 480.0 | 429.7 | |
| 0.00 | 1.96 | 0.00 | 1.20 | 18.21 | 162.69 | 27.88 | 310.68 | 0.5879 | 852.0 | 685.0 | |
| 0.00 | 0.71 | 0.00 | 0.44 | 18.37 | 162.72 | 27.91 | 310.87 | 0.5896 | 671.0 | 535.1 | |
| 0.00 | 1.51 | 0.00 | 0.93 | 18.60 | 162.69 | 27.87 | 311.21 | 0.5912 | 649.0 | 562.1 | |
| 0.00 | 2.58 | 0.00 | 1.57 | 18.00 | 162.44 | 27.62 | 310.65 | 0.5834 | 486.0 | 524.2 | |
| 0.00 | 0.89 | 0.00 | 0.54 | 18.82 | 162.44 | 27.63 | 311.75 | 0.5905 | 646.0 | 499.9 | |
| 0.00 | 0.53 | 0.00 | 0.33 | 20.21 | 162.45 | 27.63 | 313.56 | 0.6029 | 639.0 | 482.5 | |
| 0.00 | 1.16 | 0.00 | 0.72 | 20.37 | 162.41 | 27.59 | 313.81 | 0.6039 | 710.0 | 537.0 | |
| 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. | |