| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.27 | 131.71 | 33.71 | 152.47 | -16.42 | 64.30 | -60.74 | 112.12 | 0.9041 | 159.8 | 57.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.96 | 87.10 | 2.11 | 94.07 | -16.71 | 66.57 | -58.48 | 113.11 | 0.8895 | 530.4 | 209.2 | |
| 18.12 | -1.00 | 19.57 | -1.00 | -16.41 | 66.35 | -58.69 | 112.72 | 0.8904 | 682.9 | 999999 | |
| 0.00 | 0.89 | 0.00 | 1.04 | -17.18 | 64.37 | -60.68 | 112.92 | 0.9061 | 165.0 | 152.3 | |
| 0.00 | 1.43 | 0.00 | 1.64 | -16.20 | 64.45 | -60.60 | 111.90 | 0.9035 | 371.0 | 243.4 | |
| 0.62 | 1.96 | 0.73 | 2.30 | -16.56 | 63.86 | -61.18 | 112.10 | 0.9082 | 219.1 | 155.3 | |
| 0.00 | 1.34 | 0.00 | 1.60 | -16.82 | 63.32 | -61.73 | 112.21 | 0.9123 | 95.0 | 56.9 | |
| 0.00 | 0.71 | 0.00 | 0.92 | -16.40 | 61.34 | -63.70 | 111.21 | 0.9241 | -512.0 | -515.0 | |
| 0.00 | 0.62 | 0.00 | 0.81 | -16.32 | 61.17 | -63.87 | 111.08 | 0.9250 | -564.0 | -557.6 | |
| 1.43 | 35.43 | 1.88 | 47.01 | -16.53 | 60.75 | -64.29 | 111.18 | 0.9280 | -558.9 | -213.1 | |
| 0.00 | 0.98 | 0.00 | 1.33 | -17.24 | 60.22 | -64.83 | 111.78 | 0.9324 | -341.0 | -320.8 | |
| 0.45 | -9.00 | 0.60 | -9.00 | -16.64 | 60.39 | -64.66 | 111.20 | 0.9303 | -382.0 | 999999 | |
| 6.69 | -9.00 | 8.82 | -9.00 | -16.19 | 60.60 | -64.45 | 110.79 | 0.9284 | -634.8 | 999999 | |
| 0.00 | 0.98 | 0.00 | 1.37 | -17.74 | 59.57 | -65.48 | 112.12 | 0.9369 | -138.0 | -167.9 | |
| 0.00 | 0.27 | 0.00 | 0.38 | -17.59 | 59.52 | -65.52 | 111.95 | 0.9369 | -175.0 | -152.7 | |
| 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. | |