| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.51 | 63.26 | 17.25 | 43.21 | -13.20 | 118.85 | -38.94 | 117.21 | 0.6901 | 366.4 | 87.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.47 | 34.32 | 14.40 | 23.03 | -12.94 | 119.95 | -37.83 | 117.51 | 0.6763 | 854.5 | 336.3 | |
| 0.35 | 3.43 | 0.24 | 2.33 | -13.61 | 119.47 | -38.31 | 118.11 | 0.6854 | 433.2 | -43.9 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -13.14 | 119.36 | -38.42 | 117.42 | 0.6841 | 480.0 | 339.3 | |
| 0.00 | 1.67 | 0.00 | 1.14 | -13.85 | 119.19 | -38.60 | 118.26 | 0.6900 | 428.0 | 332.7 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -13.70 | 119.10 | -38.69 | 118.00 | 0.6901 | -256.0 | -206.0 | |
| 0.00 | 0.44 | 0.00 | 0.30 | -13.05 | 119.22 | -38.56 | 117.23 | 0.6852 | 464.0 | 361.0 | |
| 0.00 | 1.14 | 0.00 | 0.78 | -12.96 | 118.80 | -38.98 | 116.85 | 0.6894 | 620.0 | 413.1 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -11.67 | 118.72 | -39.06 | 115.08 | 0.6837 | 692.0 | 563.6 | |
| 0.70 | 3.08 | 0.49 | 2.15 | -14.42 | 117.95 | -39.84 | 118.25 | 0.7067 | -803.4 | -663.0 | |
| 0.00 | 0.97 | 0.00 | 0.67 | -13.45 | 117.79 | -40.00 | 116.90 | 0.7033 | 150.0 | 209.5 | |
| 0.00 | 1.76 | 0.00 | 1.21 | -12.02 | 117.86 | -39.92 | 115.06 | 0.6953 | 535.0 | 430.5 | |
| 0.97 | 6.07 | 0.68 | 4.26 | -13.82 | 117.06 | -40.73 | 116.97 | 0.7132 | -544.5 | 218.2 | |
| 0.00 | 1.14 | 0.00 | 0.81 | -14.04 | 116.72 | -41.06 | 117.06 | 0.7179 | -726.0 | -596.6 | |
| 0.00 | 1.14 | 0.00 | 0.82 | -13.67 | 116.10 | -41.68 | 116.26 | 0.7228 | -170.0 | -311.5 | |
| 2.02 | 4.14 | 1.44 | 2.95 | -13.42 | 116.03 | -41.75 | 115.90 | 0.7224 | -683.9 | -507.6 | |
| 0.00 | 0.79 | 0.00 | 0.56 | -13.02 | 115.95 | -41.83 | 115.34 | 0.7213 | -608.0 | -560.7 | |
| 0.00 | 1.06 | 0.00 | 0.76 | -13.19 | 115.83 | -41.95 | 115.49 | 0.7234 | -448.0 | -499.5 | |
| 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. | |