| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.52 | 69.42 | 13.60 | 36.94 | 19.98 | 129.66 | 0.34 | 359.41 | 0.3662 | -81.3 | -3.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.94 | 24.08 | 3.72 | 12.88 | 20.93 | 131.63 | 2.31 | 354.32 | 0.3822 | -926.9 | -608.2 | |
| 2.89 | -1.00 | 1.54 | -1.00 | 20.60 | 131.56 | 2.24 | 354.40 | 0.3768 | -1042.8 | 999999 | |
| 3.16 | 6.04 | 1.68 | 3.22 | 20.34 | 131.17 | 1.85 | 355.32 | 0.3720 | -868.0 | -630.0 | |
| 0.00 | 1.26 | 0.00 | 0.68 | 21.23 | 130.36 | 1.04 | 357.47 | 0.3855 | -630.0 | -562.9 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 19.88 | 129.32 | 0.00 | 0.00 | 0.3633 | -89.0 | -68.6 | |
| 2.89 | 30.57 | 1.53 | 16.25 | 19.53 | 128.80 | -0.51 | 1.36 | 0.3575 | 1059.1 | 744.4 | |
| 0.00 | 1.35 | 0.00 | 0.72 | 20.57 | 128.77 | -0.55 | 1.38 | 0.3745 | -37.0 | -44.9 | |
| 0.81 | -6.00 | 0.43 | -6.00 | 20.21 | 128.51 | -0.81 | 2.07 | 0.3688 | 856.3 | 999999 | |
| 6.94 | -6.00 | 3.69 | -6.00 | 19.95 | 128.45 | -0.87 | 2.26 | 0.3646 | 972.7 | 999999 | |
| 1.89 | -6.00 | 1.01 | -6.00 | 20.31 | 128.41 | -0.91 | 2.30 | 0.3705 | 704.1 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 17.01 | 127.32 | -2.00 | 6.06 | 0.3177 | -752.0 | -612.8 | |
| 0.00 | 1.44 | 0.00 | 0.75 | 14.79 | 126.52 | -2.80 | 9.65 | 0.2826 | -977.0 | -824.1 | |
| 0.00 | 1.80 | 0.00 | 0.93 | 15.42 | 125.95 | -3.37 | 11.14 | 0.2948 | -743.0 | -569.7 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 15.46 | 123.23 | -6.09 | 19.52 | 0.3075 | 839.0 | 609.2 | |
| 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. | |