| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.52 | 161.60 | 27.32 | 174.21 | -16.48 | 64.29 | -58.56 | 112.87 | 0.8887 | 200.8 | 9.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.76 | 105.29 | 17.93 | 106.35 | -16.39 | 66.43 | -56.42 | 113.46 | 0.8732 | 684.8 | 169.2 | |
| 0.00 | 1.52 | 0.00 | 1.61 | -16.72 | 64.93 | -57.92 | 113.30 | 0.8855 | 287.0 | 214.1 | |
| 0.00 | 1.61 | 0.00 | 1.71 | -16.24 | 64.63 | -58.23 | 112.68 | 0.8865 | 435.0 | 329.3 | |
| 0.71 | 1.78 | 0.78 | 1.94 | -16.60 | 63.96 | -58.89 | 112.86 | 0.8923 | 154.9 | 122.6 | |
| 0.00 | 0.98 | 0.00 | 1.09 | -16.80 | 63.36 | -59.49 | 112.88 | 0.8970 | 200.0 | 119.3 | |
| 0.00 | 2.05 | 0.00 | 2.36 | -16.26 | 62.12 | -60.74 | 111.91 | 0.9045 | -165.0 | -214.0 | |
| 0.00 | 2.59 | 0.00 | 3.07 | -16.42 | 61.31 | -61.55 | 111.84 | 0.9103 | -573.0 | -562.1 | |
| 0.00 | 1.61 | 0.00 | 2.08 | -18.83 | 59.69 | -63.17 | 113.88 | 0.9253 | -388.0 | -349.1 | |
| 0.00 | 1.61 | 0.00 | 2.01 | -17.56 | 60.16 | -62.69 | 112.70 | 0.9200 | -493.0 | -377.1 | |
| 3.30 | 40.33 | 4.04 | 49.18 | -16.66 | 60.56 | -62.29 | 111.88 | 0.9157 | -461.3 | -253.4 | |
| 0.62 | 1.52 | 0.78 | 1.90 | -17.34 | 60.09 | -62.76 | 112.45 | 0.9200 | -373.6 | -342.2 | |
| 2.59 | -10.00 | 3.13 | -10.00 | -16.23 | 60.67 | -62.18 | 111.46 | 0.9141 | -668.4 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.91 | -17.75 | 59.62 | -63.24 | 112.75 | 0.9237 | -298.0 | -218.5 | |
| 0.54 | -10.00 | 0.66 | -10.00 | -16.52 | 60.16 | -62.69 | 111.61 | 0.9180 | -96.2 | 999999 | |
| 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. | |