| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.24 | 0.00 | 11.79 | 7.77 | 134.97 | 13.93 | 317.79 | 0.3539 | 401.7 | 381.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 0.76 | 6.77 | 142.19 | 21.15 | 303.10 | 0.4295 | -635.0 | -506.1 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 8.64 | 141.49 | 20.45 | 307.57 | 0.4376 | 610.0 | 429.5 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 8.19 | 141.01 | 19.97 | 307.39 | 0.4274 | -737.0 | -599.0 | |
| 0.00 | 0.69 | 0.00 | 0.37 | 4.48 | 140.70 | 19.66 | 300.26 | 0.3900 | -717.0 | -617.9 | |
| 0.00 | 1.12 | 0.00 | 0.59 | 7.09 | 136.25 | 15.21 | 313.03 | 0.3576 | 573.0 | 544.6 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 7.52 | 136.23 | 15.19 | 313.92 | 0.3623 | 830.0 | 689.9 | |
| 0.00 | 1.21 | 0.00 | 0.64 | 7.10 | 135.75 | 14.71 | 314.01 | 0.3519 | 851.0 | 713.8 | |
| 0.00 | 1.38 | 0.00 | 0.73 | 7.99 | 135.75 | 14.71 | 315.79 | 0.3622 | 726.0 | 562.2 | |
| 0.00 | 2.33 | 0.00 | 1.24 | 8.67 | 134.82 | 13.78 | 318.96 | 0.3601 | -793.0 | -612.9 | |
| 0.00 | 2.07 | 0.00 | 1.09 | 7.41 | 133.79 | 12.75 | 318.77 | 0.3335 | 882.0 | 753.3 | |
| 0.00 | 1.38 | 0.00 | 0.72 | 7.53 | 133.48 | 12.44 | 319.69 | 0.3317 | 942.0 | 759.2 | |
| 0.00 | 1.29 | 0.00 | 0.68 | 8.13 | 133.17 | 12.13 | 321.58 | 0.3361 | 860.0 | 764.5 | |
| 0.00 | 2.07 | 0.00 | 1.08 | 8.23 | 130.75 | 9.72 | 327.76 | 0.3145 | 907.0 | 802.0 | |
| 0.00 | 1.38 | 0.00 | 0.72 | 8.26 | 130.45 | 9.41 | 328.62 | 0.3122 | 985.0 | 835.8 | |
| 0.00 | 2.50 | 0.00 | 1.30 | 8.07 | 130.39 | 9.35 | 328.48 | 0.3090 | 742.0 | 694.0 | |
| 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. | |