| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.85 | 0.00 | 10.80 | -19.02 | 162.46 | -6.47 | 154.14 | 0.2798 | -764.6 | -600.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.42 | 0.00 | 0.74 | -22.81 | 173.30 | 4.37 | 192.96 | 0.3143 | -745.0 | -558.9 | |
| 0.00 | 1.60 | 0.00 | 0.81 | -16.99 | 170.56 | 1.63 | 187.51 | 0.2093 | -753.0 | -527.5 | |
| 0.00 | 1.69 | 0.00 | 0.88 | -23.95 | 166.54 | -2.39 | 173.29 | 0.3274 | -722.0 | -562.6 | |
| 0.00 | 0.89 | 0.00 | 0.46 | -20.32 | 164.52 | -4.41 | 164.66 | 0.2742 | -461.0 | -549.6 | |
| 0.00 | 2.93 | 0.00 | 1.46 | -9.67 | 162.69 | -6.24 | 127.01 | 0.1348 | -831.0 | -480.4 | |
| 0.00 | 0.89 | 0.00 | 0.48 | -26.39 | 161.97 | -6.96 | 163.40 | 0.3816 | -853.0 | -758.1 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -19.79 | 161.86 | -7.07 | 155.56 | 0.2811 | -909.0 | -699.7 | |
| 0.00 | 1.77 | 0.00 | 0.91 | -18.94 | 161.20 | -7.74 | 152.10 | 0.2734 | -665.0 | -545.1 | |
| 0.00 | 2.31 | 0.00 | 1.19 | -19.19 | 160.99 | -7.94 | 151.93 | 0.2786 | -806.0 | -721.7 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -19.43 | 160.75 | -8.18 | 151.68 | 0.2841 | -923.0 | -720.7 | |
| 0.00 | 1.06 | 0.00 | 0.57 | -23.48 | 158.15 | -10.78 | 151.59 | 0.3623 | -960.0 | -778.2 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -23.67 | 157.97 | -10.97 | 151.46 | 0.3663 | -652.0 | -498.2 | |
| 0.00 | 1.33 | 0.00 | 0.68 | -9.81 | 155.87 | -13.07 | 110.85 | 0.2395 | -775.0 | -629.9 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -25.38 | 154.08 | -14.85 | 146.49 | 0.4213 | -650.0 | -518.7 | |
| 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. | |