| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.53 | 18.67 | 0.31 | 11.69 | 7.98 | 337.96 | -37.61 | 86.22 | 0.6042 | -422.3 | -275.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.89 | 0.00 | 0.51 | 7.75 | 345.67 | -29.91 | 86.92 | 0.4968 | -742.0 | -624.6 | |
| 0.00 | 0.80 | 0.00 | 0.46 | 7.70 | 344.43 | -31.14 | 86.97 | 0.5153 | -662.0 | -574.6 | |
| 0.00 | 1.60 | 0.00 | 0.93 | 8.04 | 344.01 | -31.56 | 86.31 | 0.5214 | -856.0 | -688.9 | |
| 0.53 | 2.04 | 0.31 | 1.20 | 7.64 | 342.89 | -32.68 | 87.04 | 0.5380 | -862.8 | -758.9 | |
| 0.00 | 1.69 | 0.00 | 0.99 | 7.87 | 342.80 | -32.77 | 86.60 | 0.5393 | -808.0 | -714.6 | |
| 0.00 | 1.60 | 0.00 | 0.94 | 7.83 | 342.59 | -32.99 | 86.67 | 0.5424 | -643.0 | -451.7 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 8.76 | 342.46 | -33.11 | 84.96 | 0.5441 | -758.0 | -574.7 | |
| 0.00 | 0.53 | 0.00 | 0.32 | 8.09 | 342.02 | -33.56 | 86.17 | 0.5506 | -631.0 | -493.3 | |
| 0.00 | 2.58 | 0.00 | 1.59 | 7.51 | 338.87 | -36.71 | 87.07 | 0.5956 | -411.0 | -374.2 | |
| 0.00 | 0.62 | 0.00 | 0.40 | 8.50 | 336.36 | -39.22 | 85.34 | 0.6296 | -596.0 | -515.7 | |
| 0.00 | 0.98 | 0.00 | 0.68 | 8.73 | 330.33 | -45.24 | 84.82 | 0.7070 | 186.0 | 234.7 | |
| 0.00 | 1.78 | 0.00 | 1.24 | 8.89 | 330.14 | -45.44 | 84.58 | 0.7094 | 596.0 | 479.8 | |
| 0.00 | 0.89 | 0.00 | 0.64 | 7.69 | 328.23 | -47.34 | 86.16 | 0.7327 | 243.0 | 264.7 | |
| 0.00 | 1.60 | 0.00 | 1.16 | 7.44 | 328.13 | -47.44 | 86.49 | 0.7341 | 169.0 | 239.4 | |
| 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. | |