| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.00 | 0.00 | 11.35 | 14.78 | 16.42 | -0.46 | 344.32 | 0.2645 | -634.2 | -496.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.19 | 0.00 | 0.62 | 14.75 | 23.96 | 7.08 | 334.79 | 0.2811 | -717.0 | -688.1 | |
| 0.00 | 1.88 | 0.00 | 0.96 | 12.60 | 21.31 | 4.43 | 340.82 | 0.2304 | -875.0 | -730.8 | |
| 0.00 | 1.19 | 0.00 | 0.62 | 16.81 | 20.75 | 3.87 | 347.35 | 0.2962 | -932.0 | -676.6 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 18.58 | 19.67 | 2.79 | 351.73 | 0.3219 | -751.0 | -657.1 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 18.18 | 19.10 | 2.22 | 353.24 | 0.3140 | -643.0 | -477.0 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 13.24 | 18.71 | 1.83 | 352.23 | 0.2306 | -483.0 | -382.6 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 12.15 | 17.58 | 0.70 | 356.73 | 0.2102 | -879.0 | -605.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 12.63 | 17.46 | 0.58 | 357.39 | 0.2184 | -814.0 | -688.6 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 12.15 | 17.31 | 0.43 | 358.00 | 0.2100 | -1009.0 | -835.0 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 9.99 | 17.27 | 0.39 | 357.76 | 0.1728 | -978.0 | -765.8 | |
| 0.00 | 1.19 | 0.00 | 0.60 | 9.90 | 17.12 | 0.24 | 358.60 | 0.1711 | -956.0 | -799.5 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 13.15 | 16.98 | 0.10 | 359.58 | 0.2270 | -805.0 | -587.5 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 12.12 | 16.67 | -0.21 | 0.97 | 0.2094 | -801.0 | -590.2 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 14.89 | 13.19 | -3.69 | 13.69 | 0.2641 | -803.0 | -634.9 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 15.53 | 13.15 | -3.73 | 13.26 | 0.2748 | -806.0 | -630.5 | |
| 0.00 | 1.96 | 0.00 | 1.08 | 24.25 | 8.71 | -8.17 | 17.57 | 0.4311 | 742.0 | 492.9 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 19.95 | 358.81 | -18.07 | 40.63 | 0.4496 | 729.0 | 574.4 | |
| 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. | |