| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.64 | 143.00 | 41.02 | 292.28 | 5.67 | 11.19 | 75.17 | 277.68 | 0.9716 | 86.2 | 88.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.39 | 0.00 | 3.12 | 2.96 | 12.69 | 76.67 | 274.70 | 0.9760 | 223.0 | 207.9 | |
| 2.09 | 11.99 | 5.31 | 30.41 | 6.34 | 13.82 | 77.80 | 277.95 | 0.9818 | -240.1 | -160.3 | |
| 0.00 | 0.96 | 0.00 | 2.10 | 3.20 | 12.48 | 76.47 | 274.98 | 0.9754 | -236.0 | -204.7 | |
| 3.13 | 7.82 | 6.96 | 17.47 | 3.72 | 12.49 | 76.47 | 275.50 | 0.9757 | -370.4 | -187.3 | |
| 0.00 | 2.69 | 0.00 | 5.92 | 4.72 | 12.29 | 76.27 | 276.55 | 0.9755 | -296.0 | -288.6 | |
| 0.00 | 3.56 | 0.00 | 7.37 | 2.89 | 11.66 | 75.64 | 274.78 | 0.9720 | -471.0 | -397.5 | |
| 0.00 | 2.61 | 0.00 | 5.59 | 4.91 | 11.85 | 75.83 | 276.81 | 0.9739 | -124.0 | -196.5 | |
| 1.30 | 7.99 | 2.76 | 16.71 | 5.31 | 11.62 | 75.61 | 277.25 | 0.9733 | 20.1 | -164.3 | |
| 0.00 | 4.08 | 0.00 | 9.02 | 6.82 | 12.03 | 76.01 | 278.72 | 0.9758 | -186.0 | -198.1 | |
| 0.00 | 0.78 | 0.00 | 1.59 | 4.69 | 11.05 | 75.03 | 276.71 | 0.9706 | -430.0 | -435.8 | |
| 6.52 | 84.97 | 13.13 | 166.47 | 6.00 | 10.82 | 74.80 | 278.08 | 0.9705 | 255.3 | 269.0 | |
| 4.60 | -11.00 | 9.06 | -11.00 | 6.34 | 10.38 | 74.36 | 278.50 | 0.9689 | 490.1 | 999999 | |
| 0.87 | 14.16 | 1.59 | 26.51 | 4.49 | 9.64 | 73.62 | 276.72 | 0.9643 | 443.7 | 13.9 | |
| 1.13 | -11.00 | 2.21 | -11.00 | 6.60 | 10.26 | 74.25 | 278.78 | 0.9685 | 433.2 | 999999 | |
| 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. | |