| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.16 | 0.00 | 11.38 | -15.36 | 128.09 | 27.09 | 248.89 | 0.4726 | 590.8 | 450.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.28 | 0.00 | 1.35 | -8.40 | 134.53 | 33.54 | 264.77 | 0.5510 | 826.0 | 627.5 | |
| 0.00 | 2.37 | 0.00 | 1.39 | -15.73 | 133.20 | 32.20 | 251.13 | 0.5443 | 226.0 | 274.4 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -13.52 | 132.51 | 31.52 | 254.95 | 0.5284 | 702.0 | 468.1 | |
| 0.00 | 1.23 | 0.00 | 0.74 | -21.13 | 133.51 | 32.52 | 241.93 | 0.5704 | 676.0 | 594.6 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -15.69 | 131.69 | 30.70 | 250.58 | 0.5232 | 668.0 | 474.6 | |
| 0.00 | 2.28 | 0.00 | 1.32 | -15.46 | 131.55 | 30.55 | 250.96 | 0.5204 | 786.0 | 651.0 | |
| 0.00 | 1.31 | 0.00 | 0.76 | -16.03 | 131.06 | 30.07 | 249.67 | 0.5156 | 870.0 | 741.6 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -19.20 | 129.78 | 28.79 | 243.06 | 0.5123 | 655.0 | 512.8 | |
| 0.00 | 1.49 | 0.00 | 0.83 | -21.82 | 124.91 | 23.92 | 234.21 | 0.4659 | 850.0 | 643.7 | |
| 0.00 | 1.75 | 0.00 | 0.97 | -20.22 | 124.54 | 23.54 | 236.92 | 0.4492 | 693.0 | 509.0 | |
| 0.00 | 0.61 | 0.00 | 0.33 | -17.54 | 123.84 | 22.84 | 241.84 | 0.4216 | 483.0 | 366.9 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -11.22 | 117.95 | 16.96 | 253.42 | 0.2999 | 790.0 | 657.6 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -11.71 | 117.85 | 16.86 | 251.77 | 0.3004 | 933.0 | 779.1 | |
| 0.00 | 1.84 | 0.00 | 0.94 | -12.61 | 114.64 | 13.64 | 244.96 | 0.2552 | -887.0 | -762.6 | |
| 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. | |