| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.24 | 270.84 | 57.29 | 225.28 | -15.07 | 118.28 | -49.33 | 114.25 | 0.8040 | 195.6 | 169.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.17 | 156.23 | 6.38 | 123.05 | -15.24 | 121.36 | -46.24 | 115.72 | 0.7758 | 1106.0 | 304.3 | |
| 20.37 | -1.00 | 16.10 | -1.00 | -15.35 | 120.88 | -46.73 | 115.63 | 0.7810 | 816.4 | 999999 | |
| 5.36 | -1.00 | 4.27 | -1.00 | -15.20 | 120.32 | -47.28 | 115.20 | 0.7858 | 536.0 | 999999 | |
| 0.00 | 1.32 | 0.00 | 1.06 | -15.10 | 119.66 | -47.94 | 114.79 | 0.7918 | 450.0 | 404.5 | |
| 5.97 | 24.59 | 4.83 | 19.91 | -14.68 | 119.37 | -48.24 | 114.16 | 0.7931 | 675.5 | 465.5 | |
| 1.41 | -5.00 | 1.14 | -5.00 | -14.41 | 119.16 | -48.44 | 113.76 | 0.7941 | 758.2 | 999999 | |
| 2.81 | 3.42 | 2.32 | 2.83 | -15.11 | 118.48 | -49.12 | 114.29 | 0.8031 | 460.1 | 408.1 | |
| 0.00 | 1.23 | 0.00 | 1.02 | -15.17 | 118.17 | -49.43 | 114.24 | 0.8062 | 253.0 | 194.4 | |
| 0.00 | 1.76 | 0.00 | 1.45 | -13.50 | 117.96 | -49.64 | 112.19 | 0.8025 | -577.0 | -453.2 | |
| 0.00 | 3.60 | 0.00 | 3.08 | -14.53 | 116.67 | -50.93 | 112.90 | 0.8180 | -647.0 | -502.6 | |
| 0.00 | 1.23 | 0.00 | 1.06 | -14.85 | 116.37 | -51.23 | 113.15 | 0.8218 | -490.0 | -500.8 | |
| 3.07 | 5.71 | 2.69 | 4.99 | -15.11 | 115.98 | -51.62 | 113.30 | 0.8262 | -481.5 | -575.4 | |
| 3.60 | 4.39 | 3.33 | 4.07 | -15.57 | 113.75 | -53.85 | 113.00 | 0.8471 | -402.1 | -169.9 | |
| 17.48 | 67.36 | 16.23 | 62.76 | -14.78 | 113.36 | -54.25 | 111.97 | 0.8482 | -730.4 | -84.4 | |
| 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. | |