| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.06 | 64.09 | 21.69 | 53.01 | -22.71 | 138.55 | -46.81 | 122.87 | 0.8015 | -23.0 | 105.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.81 | 0.00 | 2.13 | -21.77 | 142.89 | -42.47 | 123.97 | 0.7584 | 792.0 | 628.7 | |
| 4.72 | 24.24 | 3.70 | 19.00 | -22.70 | 141.30 | -44.06 | 124.19 | 0.7778 | 861.7 | 522.2 | |
| 4.27 | -2.00 | 3.34 | -2.00 | -22.36 | 141.30 | -44.06 | 123.80 | 0.7761 | 831.6 | 999999 | |
| 3.99 | 6.26 | 3.19 | 5.00 | -22.10 | 140.06 | -45.30 | 122.85 | 0.7861 | 666.3 | 455.1 | |
| 0.00 | 1.82 | 0.00 | 1.46 | -22.32 | 139.73 | -45.63 | 122.94 | 0.7901 | 302.0 | 224.9 | |
| 0.00 | 0.82 | 0.00 | 0.65 | -21.21 | 139.57 | -45.79 | 121.58 | 0.7866 | 531.0 | 418.3 | |
| 0.00 | 1.36 | 0.00 | 1.12 | -22.51 | 138.74 | -46.62 | 122.67 | 0.7998 | 364.0 | 233.3 | |
| 5.90 | 7.17 | 4.98 | 6.05 | -22.26 | 137.29 | -48.07 | 121.70 | 0.8114 | -752.3 | -573.7 | |
| 3.00 | 3.99 | 2.59 | 3.45 | -22.75 | 136.40 | -48.95 | 121.86 | 0.8210 | -685.8 | -666.5 | |
| 0.00 | 0.91 | 0.00 | 0.78 | -22.56 | 136.25 | -49.11 | 121.57 | 0.8216 | -515.0 | -453.7 | |
| 0.00 | 3.45 | 0.00 | 3.03 | -22.86 | 135.69 | -49.67 | 121.67 | 0.8274 | -753.0 | -594.1 | |
| 0.00 | 2.00 | 0.00 | 1.80 | -23.77 | 134.91 | -50.45 | 122.33 | 0.8372 | -533.0 | -565.4 | |
| 0.00 | 0.91 | 0.00 | 0.82 | -23.94 | 134.81 | -50.54 | 122.48 | 0.8387 | -425.0 | -380.9 | |
| 0.00 | 0.91 | 0.00 | 0.81 | -23.35 | 135.02 | -50.33 | 121.92 | 0.8347 | -555.0 | -428.9 | |
| 0.00 | 1.63 | 0.00 | 1.52 | -24.69 | 133.86 | -51.50 | 122.90 | 0.8489 | -299.0 | -269.1 | |
| 0.00 | 0.73 | 0.00 | 0.66 | -23.45 | 134.55 | -50.80 | 121.83 | 0.8389 | -459.0 | -453.0 | |
| 4.18 | 5.08 | 3.89 | 4.73 | -23.82 | 133.49 | -51.87 | 121.80 | 0.8487 | -454.8 | -276.6 | |
| 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. | |