| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.23 | 377.25 | 52.42 | 323.45 | 27.62 | 54.84 | 52.68 | 300.19 | 0.8171 | -810.1 | -213.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.44 | 365.57 | 46.79 | 314.46 | 27.60 | 55.12 | 52.96 | 300.07 | 0.8196 | -989.2 | -220.7 | |
| 0.70 | -1.00 | 0.59 | -1.00 | 28.07 | 54.55 | 52.39 | 300.77 | 0.8158 | -924.1 | 999999 | |
| 2.26 | -1.00 | 1.90 | -1.00 | 27.55 | 53.92 | 51.77 | 300.33 | 0.8090 | -834.9 | 999999 | |
| 2.35 | -1.00 | 1.95 | -1.00 | 27.32 | 53.55 | 51.39 | 300.15 | 0.8051 | -800.6 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.77 | 30.85 | 55.37 | 53.22 | 303.82 | 0.8299 | 198.0 | 204.9 | |
| 1.48 | 3.57 | 1.19 | 2.86 | 27.52 | 51.66 | 49.50 | 300.94 | 0.7885 | -695.9 | -657.8 | |
| 0.00 | 1.05 | 0.00 | 0.88 | 29.96 | 53.22 | 51.07 | 303.40 | 0.8095 | 502.0 | 415.6 | |
| 0.00 | 0.70 | 0.00 | 0.56 | 27.79 | 51.56 | 49.41 | 301.30 | 0.7885 | -568.0 | -527.0 | |
| 0.00 | 0.96 | 0.00 | 0.81 | 31.43 | 52.92 | 50.77 | 305.24 | 0.8114 | -593.0 | -452.8 | |
| 0.00 | 0.96 | 0.00 | 0.67 | 24.77 | 44.67 | 42.52 | 299.87 | 0.7100 | 545.0 | 409.3 | |
| 0.00 | 1.13 | 0.00 | 0.80 | 27.04 | 44.47 | 42.31 | 302.97 | 0.7170 | 677.0 | 569.4 | |
| 0.00 | 0.96 | 0.00 | 0.65 | 30.22 | 40.31 | 38.15 | 309.19 | 0.6911 | 502.0 | 440.1 | |
| 0.00 | 1.48 | 0.00 | 0.99 | 30.48 | 38.64 | 36.48 | 310.51 | 0.6764 | 593.0 | 491.2 | |
| 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. | |