| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.89 | 25.95 | 3.24 | 14.18 | -18.09 | 121.97 | 20.93 | 233.99 | 0.4219 | -187.9 | -151.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.25 | 0.00 | 0.69 | -17.30 | 123.86 | 22.81 | 237.80 | 0.4393 | 574.0 | 554.2 | |
| 3.21 | 4.91 | 1.77 | 2.70 | -17.02 | 123.72 | 22.67 | 238.21 | 0.4354 | 853.8 | 721.5 | |
| 0.00 | 2.76 | 0.00 | 1.52 | -17.49 | 123.64 | 22.60 | 237.19 | 0.4379 | 859.0 | 729.0 | |
| 2.68 | 4.19 | 1.47 | 2.30 | -17.10 | 123.15 | 22.10 | 237.46 | 0.4284 | 917.3 | 832.7 | |
| 0.00 | 3.21 | 0.00 | 1.75 | -18.80 | 121.28 | 20.24 | 231.83 | 0.4183 | -730.0 | -670.9 | |
| 0.00 | 1.07 | 0.00 | 0.58 | -18.31 | 120.54 | 19.50 | 231.85 | 0.4047 | -756.0 | -619.8 | |
| 0.00 | 1.07 | 0.00 | 0.58 | -20.23 | 120.41 | 19.36 | 227.90 | 0.4211 | -653.0 | -485.6 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -19.17 | 120.21 | 19.16 | 229.67 | 0.4084 | -901.0 | -801.7 | |
| 0.00 | 1.69 | 0.00 | 0.91 | -18.20 | 120.09 | 19.05 | 231.48 | 0.3980 | -874.0 | -657.2 | |
| 0.00 | 1.07 | 0.00 | 0.58 | -18.49 | 119.79 | 18.75 | 230.46 | 0.3969 | -830.0 | -657.0 | |
| 0.00 | 0.89 | 0.00 | 0.49 | -21.09 | 120.08 | 19.03 | 225.85 | 0.4258 | -587.0 | -462.4 | |
| 0.00 | 1.34 | 0.00 | 0.72 | -19.08 | 119.76 | 18.71 | 229.21 | 0.4022 | -900.0 | -751.3 | |
| 0.00 | 1.25 | 0.00 | 0.68 | -19.27 | 119.61 | 18.57 | 228.62 | 0.4023 | -737.0 | -588.7 | |
| 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. | |