| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.35 | 0.00 | 9.68 | -14.36 | 299.22 | -25.41 | 111.55 | 0.4461 | -514.5 | -407.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.15 | 0.00 | 0.58 | -14.06 | 318.29 | -6.34 | 142.72 | 0.1776 | 661.0 | 435.6 | |
| 0.00 | 1.76 | 0.00 | 0.91 | -8.57 | 307.71 | -16.92 | 99.72 | 0.2932 | 715.0 | 521.8 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -16.45 | 300.38 | -24.25 | 115.77 | 0.4392 | -684.0 | -603.4 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -15.35 | 300.42 | -24.21 | 113.42 | 0.4327 | -717.0 | -527.9 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -15.50 | 300.23 | -24.40 | 113.60 | 0.4362 | -697.0 | -545.8 | |
| 0.00 | 1.06 | 0.00 | 0.59 | -14.69 | 298.54 | -26.08 | 110.77 | 0.4567 | -726.0 | -457.7 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -15.12 | 298.00 | -26.63 | 111.35 | 0.4664 | -637.0 | -523.4 | |
| 0.00 | 1.85 | 0.00 | 1.06 | -16.70 | 296.39 | -28.24 | 113.54 | 0.4963 | -668.0 | -573.0 | |
| 0.00 | 1.32 | 0.00 | 0.76 | -16.82 | 295.80 | -28.83 | 113.43 | 0.5051 | -843.0 | -657.3 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -14.29 | 295.97 | -28.65 | 108.62 | 0.4923 | -784.0 | -599.5 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -16.75 | 295.56 | -29.07 | 113.16 | 0.5080 | -507.0 | -406.1 | |
| 0.00 | 2.20 | 0.00 | 1.25 | -11.87 | 296.14 | -28.48 | 103.80 | 0.4825 | -885.0 | -715.7 | |
| 0.00 | 1.41 | 0.00 | 0.82 | -13.86 | 294.15 | -30.48 | 107.02 | 0.5170 | -748.0 | -555.0 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -15.65 | 293.24 | -31.38 | 109.97 | 0.5356 | -683.0 | -444.6 | |
| 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. | |