| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.33 | 0.00 | 11.43 | 6.32 | 262.92 | -9.30 | 97.42 | 0.2165 | 499.0 | 380.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.68 | -0.35 | 279.06 | 6.84 | 242.43 | 0.1349 | -907.0 | -751.7 | |
| 0.00 | 2.54 | 0.00 | 1.26 | 4.02 | 276.60 | 4.38 | 280.37 | 0.0777 | -854.0 | -675.4 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 3.19 | 270.97 | -1.25 | 92.23 | 0.0219 | -808.0 | -583.3 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 8.92 | 269.76 | -2.46 | 23.14 | 0.1083 | 875.0 | 790.1 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 8.65 | 269.67 | -2.55 | 24.98 | 0.1046 | 771.0 | 646.9 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 8.86 | 269.61 | -2.61 | 24.66 | 0.1084 | 917.0 | 722.8 | |
| 0.00 | 2.00 | 0.00 | 1.00 | 11.81 | 268.03 | -4.19 | 25.63 | 0.1662 | 917.0 | 667.0 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 12.11 | 266.62 | -5.60 | 31.71 | 0.1824 | 922.0 | 737.6 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 1.61 | 260.12 | -12.10 | 97.40 | 0.2122 | 962.0 | 739.7 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 7.24 | 259.25 | -12.97 | 72.27 | 0.2348 | 961.0 | 740.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 6.61 | 255.91 | -16.32 | 77.64 | 0.2869 | 718.0 | 569.1 | |
| 0.00 | 2.36 | 0.00 | 1.26 | 5.71 | 250.98 | -21.24 | 82.59 | 0.3651 | 842.0 | 694.2 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 7.72 | 250.79 | -21.43 | 77.24 | 0.3728 | 583.0 | 474.9 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 6.73 | 250.11 | -22.11 | 80.13 | 0.3810 | 646.0 | 491.4 | |
| 0.00 | 2.45 | 0.00 | 1.32 | 4.54 | 249.30 | -22.92 | 85.98 | 0.3908 | 940.0 | 777.9 | |
| 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. | |