| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.82 | 0.00 | 12.15 | -22.96 | 74.68 | -15.01 | 153.82 | 0.5161 | 337.0 | 291.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.30 | 0.00 | 0.75 | -26.10 | 84.63 | -5.05 | 171.05 | 0.5100 | -697.0 | -572.1 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -20.34 | 84.06 | -5.62 | 167.44 | 0.4243 | 704.0 | 411.6 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -28.29 | 81.40 | -8.28 | 166.64 | 0.5510 | -711.0 | -574.1 | |
| 0.00 | 2.85 | 0.00 | 1.57 | -20.73 | 80.94 | -8.75 | 161.22 | 0.4435 | 736.0 | 649.2 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -17.82 | 77.60 | -12.08 | 151.75 | 0.4227 | 675.0 | 419.7 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -20.48 | 77.24 | -12.44 | 153.97 | 0.4619 | 740.0 | 559.3 | |
| 0.00 | 1.64 | 0.00 | 0.92 | -20.49 | 76.75 | -12.93 | 153.11 | 0.4654 | 573.0 | 528.3 | |
| 0.00 | 2.51 | 0.00 | 1.40 | -20.33 | 76.14 | -13.54 | 151.88 | 0.4677 | 819.0 | 614.7 | |
| 0.00 | 2.33 | 0.00 | 1.31 | -20.70 | 76.04 | -13.64 | 152.09 | 0.4732 | 764.0 | 635.5 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -22.13 | 73.44 | -16.24 | 149.42 | 0.5111 | 689.0 | 474.3 | |
| 0.00 | 1.21 | 0.00 | 0.72 | -24.46 | 72.26 | -17.42 | 150.10 | 0.5490 | 695.0 | 603.3 | |
| 0.00 | 0.86 | 0.00 | 0.53 | -25.72 | 69.13 | -20.55 | 147.28 | 0.5873 | 583.0 | 511.0 | |
| 0.00 | 0.95 | 0.00 | 0.66 | -28.88 | 58.37 | -31.32 | 139.58 | 0.7043 | -646.0 | -561.5 | |
| 0.00 | 1.47 | 0.00 | 1.08 | -29.59 | 54.76 | -34.92 | 137.47 | 0.7388 | -206.0 | -277.9 | |
| 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. | |