| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.27 | 50.50 | 11.21 | 26.56 | 17.97 | 315.59 | 11.52 | 326.02 | 0.3356 | -416.5 | -122.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 0.69 | 17.84 | 321.99 | 17.91 | 312.78 | 0.4005 | 805.0 | 635.7 | |
| 0.00 | 3.17 | 0.00 | 1.69 | 18.68 | 318.95 | 14.87 | 319.47 | 0.3757 | -790.0 | -694.9 | |
| 6.26 | 7.72 | 3.33 | 4.11 | 18.78 | 318.02 | 13.94 | 321.41 | 0.3673 | -931.6 | -773.4 | |
| 0.00 | 2.40 | 0.00 | 1.27 | 18.20 | 317.75 | 13.67 | 320.88 | 0.3574 | -931.0 | -853.2 | |
| 0.86 | 2.23 | 0.46 | 1.18 | 18.60 | 317.68 | 13.60 | 321.75 | 0.3616 | -816.9 | -835.8 | |
| 9.52 | 15.35 | 5.01 | 8.08 | 17.90 | 316.57 | 12.49 | 322.76 | 0.3417 | -1066.3 | -470.5 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 17.97 | 315.62 | 11.54 | 325.00 | 0.3334 | 731.0 | 527.2 | |
| 1.80 | 1.80 | 0.95 | 0.95 | 18.65 | 315.54 | 11.46 | 326.38 | 0.3416 | 763.8 | 0.0 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 18.00 | 315.27 | 11.20 | 325.86 | 0.3306 | 742.0 | 617.2 | |
| 0.00 | 4.55 | 0.00 | 2.38 | 18.13 | 315.00 | 10.92 | 326.74 | 0.3297 | 1052.0 | 899.6 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.31 | 311.99 | 7.91 | 333.22 | 0.2931 | -899.0 | -709.7 | |
| 2.40 | 2.57 | 1.24 | 1.33 | 16.73 | 311.50 | 7.42 | 333.74 | 0.2808 | -900.2 | -751.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 18.24 | 309.99 | 5.91 | 340.48 | 0.2942 | -981.0 | -698.4 | |
| 0.43 | 1.46 | 0.22 | 0.76 | 18.40 | 309.56 | 5.48 | 341.98 | 0.2943 | -830.6 | -641.2 | |
| 0.00 | 1.80 | 0.00 | 0.91 | 13.44 | 307.04 | 2.97 | 345.48 | 0.2017 | 850.0 | 728.4 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 17.39 | 306.73 | 2.65 | 350.42 | 0.2664 | 795.0 | 582.8 | |
| 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. | |