| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.63 | 36.52 | 5.67 | 19.43 | -14.97 | 4.19 | 5.89 | 195.59 | 0.3662 | -124.7 | -49.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.53 | 0.00 | 1.35 | -14.87 | 6.26 | 7.96 | 201.07 | 0.3740 | 938.0 | 683.7 | |
| 4.88 | 6.71 | 2.60 | 3.57 | -14.58 | 6.12 | 7.83 | 201.03 | 0.3688 | 1019.6 | 808.2 | |
| 3.31 | 8.19 | 1.78 | 4.41 | -16.24 | 6.03 | 7.73 | 199.25 | 0.3935 | 1001.6 | 725.4 | |
| 0.00 | 0.96 | 0.00 | 0.52 | -17.18 | 5.91 | 7.61 | 198.20 | 0.4070 | -752.0 | -602.5 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -17.27 | 5.47 | 7.18 | 197.15 | 0.4063 | -887.0 | -723.6 | |
| 0.96 | 1.92 | 0.51 | 1.02 | -15.07 | 4.55 | 6.26 | 196.68 | 0.3681 | 702.3 | 850.4 | |
| 0.00 | 1.13 | 0.00 | 0.60 | -15.22 | 3.94 | 5.64 | 195.00 | 0.3678 | 675.0 | 564.9 | |
| 0.00 | 1.48 | 0.00 | 0.78 | -13.53 | 2.63 | 4.33 | 192.69 | 0.3357 | -680.0 | -392.8 | |
| 0.00 | 1.66 | 0.00 | 0.88 | -14.54 | 2.15 | 3.86 | 190.75 | 0.3504 | -791.0 | -563.5 | |
| 0.00 | 1.57 | 0.00 | 0.82 | -13.21 | 1.92 | 3.62 | 190.84 | 0.3281 | -909.0 | -698.1 | |
| 0.00 | 1.22 | 0.00 | 0.64 | -13.62 | 1.89 | 3.59 | 190.53 | 0.3347 | -1092.0 | -831.9 | |
| 0.00 | 1.74 | 0.00 | 0.92 | -14.28 | 1.87 | 3.57 | 190.11 | 0.3454 | -860.0 | -641.8 | |
| 0.00 | 1.92 | 0.00 | 1.01 | -13.97 | 1.71 | 3.41 | 189.83 | 0.3398 | -945.0 | -656.5 | |
| 1.48 | 2.96 | 0.78 | 1.56 | -13.58 | 1.06 | 2.76 | 188.15 | 0.3319 | -946.9 | -834.4 | |
| 0.00 | 1.66 | 0.00 | 0.88 | -16.16 | 0.07 | 1.77 | 184.59 | 0.3721 | -829.0 | -696.4 | |
| 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. | |