| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.02 | 279.62 | 29.57 | 179.43 | -18.38 | 352.15 | 36.22 | 241.77 | 0.6387 | 940.2 | 397.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.96 | 0.00 | 1.29 | -19.07 | 354.04 | 38.11 | 241.82 | 0.6642 | -664.0 | -465.7 | |
| 5.70 | 18.88 | 3.69 | 12.26 | -19.24 | 352.51 | 36.58 | 240.75 | 0.6473 | 643.0 | 219.5 | |
| 38.53 | 242.69 | 24.74 | 155.71 | -18.22 | 352.22 | 36.29 | 242.06 | 0.6387 | 1157.2 | 405.9 | |
| 0.00 | 1.02 | 0.00 | 0.64 | -17.90 | 350.80 | 34.87 | 241.75 | 0.6200 | 715.0 | 602.9 | |
| 0.00 | 1.11 | 0.00 | 0.71 | -20.16 | 351.24 | 35.31 | 238.69 | 0.6374 | 382.0 | 293.8 | |
| 0.60 | 3.57 | 0.38 | 2.28 | -20.04 | 351.05 | 35.13 | 238.75 | 0.6346 | 827.0 | 615.3 | |
| 0.00 | 1.19 | 0.00 | 0.75 | -18.33 | 350.56 | 34.63 | 240.95 | 0.6194 | 702.0 | 629.9 | |
| 1.19 | 1.79 | 0.76 | 1.14 | -19.54 | 350.77 | 34.85 | 239.30 | 0.6285 | 733.1 | 676.0 | |
| 0.00 | 1.62 | 0.00 | 1.03 | -20.48 | 350.93 | 35.01 | 238.05 | 0.6357 | 624.0 | 458.4 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -20.16 | 350.78 | 34.85 | 238.40 | 0.6321 | 706.0 | 599.1 | |
| 0.00 | 1.70 | 0.00 | 1.08 | -19.70 | 350.58 | 34.66 | 238.95 | 0.6272 | 831.0 | 670.0 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -19.51 | 350.19 | 34.27 | 238.98 | 0.6216 | 806.0 | 682.7 | |
| 0.00 | 0.85 | 0.00 | 0.53 | -20.59 | 349.10 | 33.17 | 236.68 | 0.6152 | 701.0 | 579.8 | |
| 0.00 | 1.28 | 0.00 | 0.77 | -20.84 | 345.71 | 29.78 | 233.76 | 0.5778 | 640.0 | 467.4 | |
| 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. | |