| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.61 | 315.93 | 25.61 | 170.10 | 5.87 | 44.90 | -20.59 | 70.85 | 0.3924 | -947.0 | -372.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.74 | 9.67 | 65.54 | 0.05 | 359.78 | 0.2385 | -810.0 | -625.8 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 12.33 | 59.11 | -6.38 | 21.07 | 0.3034 | -910.0 | -756.2 | |
| 0.00 | 3.83 | 0.00 | 1.98 | 10.93 | 58.26 | -7.23 | 25.57 | 0.2875 | -515.0 | -506.8 | |
| 0.00 | 3.06 | 0.00 | 1.59 | 8.90 | 53.15 | -12.33 | 43.45 | 0.3083 | -845.0 | -619.7 | |
| 0.00 | 5.10 | 0.00 | 2.66 | 9.57 | 52.92 | -12.57 | 42.51 | 0.3191 | -694.0 | -749.7 | |
| 0.00 | 1.11 | 0.00 | 0.59 | 12.21 | 49.13 | -16.36 | 44.78 | 0.3926 | -786.0 | -529.7 | |
| 0.00 | 1.79 | 0.00 | 0.97 | 12.32 | 48.27 | -17.22 | 46.03 | 0.4036 | -587.0 | -454.3 | |
| 0.00 | 2.21 | 0.00 | 1.19 | 11.83 | 48.27 | -17.22 | 46.94 | 0.3983 | -949.0 | -777.2 | |
| 0.00 | 2.64 | 0.00 | 1.47 | 15.09 | 46.22 | -19.26 | 44.48 | 0.4565 | -874.0 | -729.1 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -0.65 | 46.46 | -19.03 | 80.30 | 0.3322 | 843.0 | 703.9 | |
| 45.99 | 282.05 | 24.74 | 151.81 | 5.49 | 44.55 | -20.94 | 65.61 | 0.3923 | -1426.8 | -389.5 | |
| 1.62 | -11.00 | 0.87 | -11.00 | 5.29 | 44.02 | -21.47 | 66.61 | 0.3989 | -724.8 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 3.41 | 40.11 | -25.38 | 73.93 | 0.4472 | 914.0 | 755.4 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 14.07 | 38.81 | -26.68 | 55.08 | 0.5332 | -682.0 | -595.6 | |
| 0.00 | 1.45 | 0.00 | 0.80 | -0.70 | 39.03 | -26.45 | 83.43 | 0.4503 | 762.0 | 457.8 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 6.21 | 38.54 | -26.95 | 69.25 | 0.4837 | 710.0 | 483.0 | |
| 0.00 | 3.32 | 0.00 | 1.90 | 7.20 | 37.51 | -27.98 | 68.09 | 0.5037 | 223.0 | 346.0 | |
| 0.00 | 2.64 | 0.00 | 1.52 | 7.02 | 36.85 | -28.64 | 68.90 | 0.5120 | 722.0 | 579.1 | |
| 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. | |