| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.36 | 289.83 | 30.46 | 169.17 | -23.87 | 193.10 | -24.67 | 133.84 | 0.5306 | 728.0 | 320.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.36 | 276.79 | 8.90 | 160.94 | -23.60 | 193.86 | -23.92 | 134.21 | 0.5203 | 1264.1 | 370.4 | |
| 0.27 | -1.00 | 0.16 | -1.00 | -24.21 | 193.55 | -24.22 | 134.79 | 0.5293 | 704.7 | 999999 | |
| 10.06 | -1.00 | 5.84 | -1.00 | -23.52 | 193.51 | -24.26 | 133.72 | 0.5234 | 1208.0 | 999999 | |
| 23.53 | -1.00 | 13.72 | -1.00 | -23.88 | 193.25 | -24.52 | 133.97 | 0.5293 | 1003.2 | 999999 | |
| 3.14 | -1.00 | 1.84 | -1.00 | -23.80 | 192.72 | -25.05 | 133.30 | 0.5344 | 508.8 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -23.26 | 191.62 | -26.15 | 131.37 | 0.5416 | 710.0 | 537.2 | |
| 0.00 | 1.71 | 0.00 | 1.05 | -25.35 | 188.30 | -29.47 | 131.36 | 0.5946 | -760.0 | -673.9 | |
| 0.00 | 1.08 | 0.00 | 0.70 | -29.41 | 185.60 | -32.18 | 134.55 | 0.6532 | -534.0 | -473.5 | |
| 0.00 | 1.62 | 0.00 | 1.02 | -26.23 | 186.44 | -31.33 | 131.06 | 0.6208 | -221.0 | -339.3 | |
| 0.00 | 1.98 | 0.00 | 1.24 | -25.93 | 186.37 | -31.40 | 130.60 | 0.6193 | -917.0 | -716.7 | |
| 0.00 | 0.72 | 0.00 | 0.46 | -26.25 | 185.92 | -31.85 | 130.68 | 0.6264 | -613.0 | -549.2 | |
| 0.00 | 3.14 | 0.00 | 2.01 | -26.51 | 185.36 | -32.41 | 130.60 | 0.6340 | -664.0 | -553.0 | |
| 0.00 | 0.81 | 0.00 | 0.53 | -27.45 | 184.07 | -33.70 | 130.89 | 0.6537 | -691.0 | -598.1 | |
| 0.00 | 0.90 | 0.00 | 0.59 | -28.11 | 183.67 | -34.10 | 131.47 | 0.6623 | -676.0 | -488.1 | |
| 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. | |