| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.80 | 22.57 | 0.47 | 13.84 | 8.11 | 340.61 | -36.06 | 86.11 | 0.5836 | -556.0 | -450.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.31 | 0.00 | 1.33 | 7.93 | 345.65 | -31.02 | 86.54 | 0.5134 | -686.0 | -605.4 | |
| 0.00 | 2.58 | 0.00 | 1.51 | 8.01 | 344.07 | -32.61 | 86.35 | 0.5368 | -750.0 | -619.7 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 8.14 | 343.76 | -32.91 | 86.10 | 0.5412 | -670.0 | -516.8 | |
| 0.00 | 1.15 | 0.00 | 0.68 | 6.52 | 343.42 | -33.25 | 89.07 | 0.5469 | -602.0 | -357.1 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 7.86 | 343.10 | -33.58 | 86.60 | 0.5509 | -725.0 | -580.3 | |
| 0.80 | 1.78 | 0.47 | 1.06 | 7.63 | 342.90 | -33.78 | 87.00 | 0.5539 | -859.6 | -771.5 | |
| 0.00 | 1.60 | 0.00 | 0.95 | 7.81 | 342.84 | -33.83 | 86.68 | 0.5546 | -667.0 | -607.9 | |
| 0.00 | 1.15 | 0.00 | 0.69 | 7.29 | 342.78 | -33.89 | 87.61 | 0.5558 | -701.0 | -539.9 | |
| 0.00 | 0.89 | 0.00 | 0.53 | 7.95 | 342.72 | -33.95 | 86.42 | 0.5563 | -559.0 | -446.5 | |
| 0.00 | 1.33 | 0.00 | 0.79 | 8.75 | 342.53 | -34.14 | 84.97 | 0.5590 | -734.0 | -561.0 | |
| 0.00 | 0.89 | 0.00 | 0.53 | 7.82 | 342.51 | -34.16 | 86.65 | 0.5594 | -575.0 | -484.7 | |
| 0.00 | 0.98 | 0.00 | 0.59 | 8.17 | 341.92 | -34.75 | 86.01 | 0.5677 | -565.0 | -502.1 | |
| 0.00 | 1.33 | 0.00 | 0.83 | 9.41 | 339.41 | -37.27 | 83.87 | 0.6030 | -563.0 | -488.1 | |
| 0.00 | 1.33 | 0.00 | 0.83 | 7.51 | 338.73 | -37.94 | 86.99 | 0.6126 | -695.0 | -587.7 | |
| 0.00 | 0.89 | 0.00 | 0.58 | 9.40 | 335.77 | -40.90 | 83.90 | 0.6519 | -551.0 | -464.6 | |
| 0.00 | 0.98 | 0.00 | 0.73 | 7.41 | 328.09 | -48.58 | 86.46 | 0.7474 | 344.0 | 276.5 | |
| 0.00 | 1.24 | 0.00 | 0.95 | 10.12 | 326.57 | -50.10 | 82.79 | 0.7636 | 250.0 | 261.4 | |
| 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. | |