| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.39 | 380.56 | 38.33 | 204.48 | -16.29 | 12.38 | 19.89 | 237.64 | 0.3883 | 1017.1 | 420.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.76 | 0.00 | 0.42 | -15.42 | 14.91 | 22.42 | 242.30 | 0.4171 | -695.0 | -527.7 | |
| 29.66 | 219.37 | 16.03 | 118.57 | -16.55 | 13.22 | 20.73 | 238.06 | 0.4016 | 1236.4 | 402.7 | |
| 3.91 | -2.00 | 2.11 | -2.00 | -16.56 | 12.83 | 20.34 | 237.59 | 0.3964 | 1366.8 | 999999 | |
| 5.01 | -2.00 | 2.70 | -2.00 | -16.69 | 12.58 | 20.09 | 237.02 | 0.3940 | 1131.9 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.77 | -16.34 | 11.99 | 19.50 | 237.08 | 0.3833 | 289.0 | 337.1 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -16.16 | 11.97 | 19.48 | 237.47 | 0.3816 | 470.0 | 445.7 | |
| 0.51 | 2.80 | 0.27 | 1.49 | -14.93 | 11.79 | 19.30 | 240.16 | 0.3698 | -416.0 | -78.8 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -18.85 | 12.14 | 19.65 | 231.84 | 0.4065 | 800.0 | 610.3 | |
| 0.00 | 2.80 | 0.00 | 1.50 | -16.77 | 11.84 | 19.35 | 235.92 | 0.3847 | 863.0 | 600.7 | |
| 0.00 | 2.12 | 0.00 | 1.13 | -14.79 | 11.42 | 18.93 | 240.07 | 0.3635 | 955.0 | 754.3 | |
| 32.30 | 145.25 | 17.22 | 77.39 | -15.84 | 11.45 | 18.96 | 237.57 | 0.3720 | 1300.7 | 465.5 | |
| 0.00 | 0.93 | 0.00 | 0.50 | -19.18 | 11.25 | 18.76 | 229.97 | 0.3985 | 736.0 | 667.2 | |
| 0.00 | 0.68 | 0.00 | 0.37 | -21.49 | 10.81 | 18.32 | 224.87 | 0.4163 | 760.0 | 626.5 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -17.80 | 3.69 | 11.20 | 218.89 | 0.2959 | -807.0 | -607.7 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -15.26 | 2.39 | 9.91 | 221.81 | 0.2501 | -828.0 | -585.6 | |
| 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. | |