| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.46 | 77.56 | 14.43 | 45.71 | -17.63 | 161.50 | 22.64 | 222.54 | 0.5447 | 660.1 | 512.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.55 | -17.26 | 165.91 | 27.05 | 228.08 | 0.5859 | 670.0 | 560.7 | |
| 0.00 | 2.98 | 0.00 | 1.79 | -18.72 | 162.56 | 23.70 | 222.47 | 0.5660 | 741.0 | 588.8 | |
| 0.00 | 0.45 | 0.00 | 0.27 | -18.67 | 162.31 | 23.45 | 222.23 | 0.5631 | 659.0 | 543.0 | |
| 21.30 | 53.96 | 12.57 | 31.79 | -17.26 | 162.04 | 23.18 | 223.72 | 0.5460 | 949.8 | 568.7 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -17.53 | 160.70 | 21.84 | 221.68 | 0.5354 | 891.0 | 673.7 | |
| 2.17 | 5.41 | 1.28 | 3.21 | -18.87 | 160.70 | 21.84 | 220.00 | 0.5498 | 862.1 | 695.5 | |
| 0.00 | 1.62 | 0.00 | 0.95 | -18.09 | 160.59 | 21.74 | 220.83 | 0.5405 | 745.0 | 611.8 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -19.02 | 160.51 | 21.65 | 219.57 | 0.5498 | 732.0 | 568.1 | |
| 0.00 | 1.62 | 0.00 | 0.96 | -18.82 | 160.38 | 21.52 | 219.65 | 0.5463 | 880.0 | 749.6 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -17.48 | 159.42 | 20.56 | 220.07 | 0.5225 | -623.0 | -567.1 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -19.49 | 159.54 | 20.68 | 217.74 | 0.5460 | 646.0 | 489.6 | |
| 0.54 | 1.71 | 0.31 | 0.99 | -17.65 | 158.76 | 19.90 | 218.94 | 0.5182 | -705.3 | -582.2 | |
| 0.00 | 1.17 | 0.00 | 0.68 | -18.54 | 158.56 | 19.70 | 217.55 | 0.5265 | 821.0 | 723.8 | |
| 0.45 | 1.71 | 0.27 | 1.03 | -21.53 | 158.85 | 19.99 | 214.52 | 0.5634 | -719.4 | -603.8 | |
| 0.00 | 1.44 | 0.00 | 0.79 | -14.42 | 154.06 | 15.20 | 215.81 | 0.4358 | 741.0 | 642.4 | |
| 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. | |