| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 27.22 | 0.00 | 14.79 | 16.43 | 25.68 | -12.38 | 29.95 | 0.4109 | -21.8 | 52.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.53 | 0.00 | 0.82 | 16.15 | 29.78 | -8.28 | 21.66 | 0.3764 | -916.0 | -733.7 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 15.81 | 29.33 | -8.73 | 23.08 | 0.3741 | -762.0 | -637.4 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 15.62 | 29.31 | -8.75 | 23.34 | 0.3714 | -799.0 | -676.4 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 15.97 | 29.23 | -8.83 | 23.14 | 0.3771 | -766.0 | -684.4 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 15.60 | 28.90 | -9.15 | 24.32 | 0.3737 | -625.0 | -544.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 16.52 | 28.24 | -9.82 | 24.79 | 0.3916 | -737.0 | -618.0 | |
| 0.00 | 2.04 | 0.00 | 1.10 | 16.46 | 27.83 | -10.22 | 25.74 | 0.3936 | -885.0 | -788.7 | |
| 0.00 | 2.30 | 0.00 | 1.24 | 16.37 | 27.50 | -10.56 | 26.58 | 0.3947 | -967.0 | -782.9 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 17.46 | 26.33 | -11.72 | 27.72 | 0.4186 | -724.0 | -469.6 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 16.90 | 24.44 | -13.62 | 32.09 | 0.4258 | 757.0 | 609.4 | |
| 0.00 | 0.94 | 0.00 | 0.51 | 16.93 | 24.22 | -13.84 | 32.46 | 0.4282 | 745.0 | 575.9 | |
| 0.00 | 1.19 | 0.00 | 0.65 | 17.28 | 24.16 | -13.90 | 32.11 | 0.4333 | 840.0 | 690.1 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 17.23 | 23.75 | -14.31 | 32.93 | 0.4360 | 715.0 | 601.8 | |
| 0.00 | 4.76 | 0.00 | 2.59 | 15.87 | 23.79 | -14.27 | 34.71 | 0.4182 | 815.0 | 806.5 | |
| 0.00 | 1.53 | 0.00 | 0.85 | 17.19 | 22.76 | -15.29 | 34.74 | 0.4441 | 771.0 | 674.3 | |
| 0.00 | 1.19 | 0.00 | 0.65 | 16.21 | 22.55 | -15.50 | 36.45 | 0.4338 | 917.0 | 783.3 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 17.04 | 22.26 | -15.79 | 35.80 | 0.4468 | 863.0 | 755.8 | |
| 0.00 | 1.87 | 0.00 | 1.04 | 16.83 | 21.70 | -16.35 | 37.03 | 0.4494 | 365.0 | 490.6 | |
| 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. | |