| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.89 | 67.63 | 25.33 | 62.97 | -21.24 | 36.64 | 55.09 | 244.53 | 0.8482 | 374.1 | 136.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.94 | 30.87 | 14.72 | 30.34 | -19.28 | 39.37 | 57.82 | 247.53 | 0.8666 | 653.6 | 320.1 | |
| 0.00 | 1.27 | 0.00 | 1.27 | -20.06 | 39.70 | 58.14 | 246.72 | 0.8706 | 371.0 | 252.9 | |
| 0.00 | 0.81 | 0.00 | 0.81 | -22.31 | 38.75 | 57.20 | 243.96 | 0.8675 | 363.0 | 316.4 | |
| 0.00 | 1.63 | 0.00 | 1.53 | -20.51 | 37.20 | 55.65 | 245.61 | 0.8511 | 572.0 | 519.3 | |
| 2.08 | 2.72 | 1.93 | 2.51 | -22.14 | 36.17 | 54.62 | 243.46 | 0.8462 | 422.6 | 302.0 | |
| 0.00 | 1.18 | 0.00 | 1.05 | -22.04 | 34.60 | 53.05 | 243.11 | 0.8326 | 550.0 | 507.5 | |
| 8.51 | 12.58 | 7.51 | 11.10 | -23.09 | 33.92 | 52.37 | 241.68 | 0.8297 | 525.9 | 361.1 | |
| 0.00 | 0.72 | 0.00 | 0.65 | -24.43 | 34.31 | 52.76 | 240.27 | 0.8368 | -304.0 | -372.9 | |
| 0.00 | 1.09 | 0.00 | 0.92 | -21.22 | 32.47 | 50.92 | 243.41 | 0.8114 | -381.0 | -394.5 | |
| 0.00 | 0.36 | 0.00 | 0.30 | -21.44 | 32.27 | 50.71 | 243.07 | 0.8102 | -562.0 | -514.5 | |
| 0.00 | 1.27 | 0.00 | 1.09 | -23.56 | 32.67 | 51.12 | 240.72 | 0.8202 | -214.0 | -54.5 | |
| 0.00 | 2.63 | 0.00 | 2.31 | -24.56 | 33.23 | 51.68 | 239.76 | 0.8281 | -421.0 | -402.7 | |
| 1.36 | 9.05 | 1.17 | 7.84 | -23.99 | 32.59 | 51.03 | 240.19 | 0.8208 | -490.7 | -148.3 | |
| 0.00 | 1.45 | 0.00 | 1.25 | -24.26 | 32.36 | 50.81 | 239.80 | 0.8197 | -571.0 | -408.2 | |
| 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. | |