| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.42 | 0.00 | 10.84 | 5.29 | 82.95 | 44.65 | 277.17 | 0.7070 | 53.8 | 74.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 0.66 | 7.19 | 88.44 | 50.14 | 279.07 | 0.7736 | -471.0 | -330.1 | |
| 0.00 | 0.94 | 0.00 | 0.71 | 0.53 | 87.16 | 48.87 | 270.42 | 0.7555 | -442.0 | -286.5 | |
| 0.00 | 1.19 | 0.00 | 0.90 | 4.55 | 86.93 | 48.63 | 275.78 | 0.7542 | -237.0 | -280.9 | |
| 0.00 | 1.11 | 0.00 | 0.82 | 8.49 | 85.87 | 47.57 | 281.14 | 0.7464 | -667.0 | -576.3 | |
| 0.00 | 0.68 | 0.00 | 0.50 | 5.01 | 85.37 | 47.07 | 276.53 | 0.7365 | -481.0 | -460.5 | |
| 0.00 | 0.77 | 0.00 | 0.57 | 7.47 | 85.63 | 47.33 | 279.83 | 0.7422 | -537.0 | -473.1 | |
| 0.00 | 1.45 | 0.00 | 1.01 | 3.89 | 82.93 | 44.63 | 275.21 | 0.7062 | 502.0 | 434.1 | |
| 0.00 | 1.02 | 0.00 | 0.71 | 2.94 | 82.58 | 44.28 | 273.88 | 0.7012 | 484.0 | 383.3 | |
| 0.00 | 0.85 | 0.00 | 0.59 | 3.24 | 82.22 | 43.93 | 274.34 | 0.6970 | 432.0 | 416.6 | |
| 0.00 | 1.11 | 0.00 | 0.77 | 5.94 | 82.27 | 43.98 | 278.20 | 0.7001 | 569.0 | 411.8 | |
| 0.00 | 1.02 | 0.00 | 0.73 | 12.35 | 82.92 | 44.62 | 287.01 | 0.7199 | -512.0 | -349.1 | |
| 0.00 | 1.11 | 0.00 | 0.73 | 4.47 | 78.89 | 40.59 | 276.48 | 0.6552 | 265.0 | 306.2 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 5.21 | 78.67 | 40.37 | 277.65 | 0.6532 | 599.0 | 515.7 | |
| 0.00 | 1.36 | 0.00 | 0.88 | 4.86 | 77.71 | 39.42 | 277.24 | 0.6401 | 657.0 | 600.8 | |
| 0.00 | 1.19 | 0.00 | 0.76 | 3.59 | 77.18 | 38.88 | 275.31 | 0.6314 | 646.0 | 564.6 | |
| 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. | |