| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.72 | 34.74 | 8.26 | 20.59 | -19.90 | 51.11 | 27.39 | 232.33 | 0.5471 | 393.2 | 204.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.78 | -19.66 | 55.92 | 32.20 | 237.20 | 0.5992 | 596.0 | 503.3 | |
| 10.93 | 13.90 | 6.62 | 8.43 | -19.54 | 54.23 | 30.51 | 236.12 | 0.5785 | 821.2 | 567.4 | |
| 0.00 | 1.17 | 0.00 | 0.71 | -19.45 | 53.88 | 30.15 | 235.99 | 0.5736 | 917.0 | 749.8 | |
| 1.26 | 3.61 | 0.76 | 2.17 | -19.03 | 53.61 | 29.88 | 236.42 | 0.5675 | 884.8 | 732.7 | |
| 0.00 | 1.35 | 0.00 | 0.79 | -14.86 | 52.49 | 28.77 | 242.45 | 0.5268 | 793.0 | 641.7 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -23.09 | 52.99 | 29.27 | 229.87 | 0.5904 | 636.0 | 489.1 | |
| 0.00 | 0.99 | 0.00 | 0.59 | -20.50 | 51.05 | 27.33 | 231.96 | 0.5482 | 636.0 | 524.5 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -16.35 | 50.18 | 26.46 | 237.96 | 0.5063 | 769.0 | 579.5 | |
| 1.53 | 3.16 | 0.88 | 1.82 | -19.58 | 48.65 | 24.93 | 231.05 | 0.5128 | -874.7 | -688.1 | |
| 0.00 | 1.63 | 0.00 | 0.96 | -23.94 | 48.63 | 24.91 | 224.46 | 0.5517 | 714.0 | 567.9 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -19.78 | 46.01 | 22.29 | 227.74 | 0.4841 | -719.0 | -569.0 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -22.03 | 42.47 | 18.75 | 219.55 | 0.4697 | -591.0 | -486.2 | |
| 0.00 | 2.62 | 0.00 | 1.46 | -22.36 | 40.75 | 17.03 | 216.50 | 0.4572 | -681.0 | -565.6 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -21.55 | 38.38 | 14.65 | 213.71 | 0.4257 | -836.0 | -686.7 | |
| 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. | |