| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.41 | 0.00 | 7.62 | -9.55 | 338.43 | -33.78 | 111.38 | 0.5902 | 154.9 | 59.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.52 | 0.00 | 0.30 | -10.13 | 342.31 | -29.90 | 114.74 | 0.5424 | 672.0 | 546.3 | |
| 0.00 | 0.60 | 0.00 | 0.35 | -9.44 | 342.24 | -29.97 | 113.50 | 0.5394 | 562.0 | 501.7 | |
| 0.00 | 1.29 | 0.00 | 0.75 | -5.85 | 341.97 | -30.24 | 106.93 | 0.5257 | 738.0 | 485.3 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -9.98 | 341.35 | -30.86 | 113.82 | 0.5544 | 539.0 | 322.6 | |
| 0.00 | 0.69 | 0.00 | 0.41 | -9.10 | 341.26 | -30.95 | 112.27 | 0.5509 | 673.0 | 508.8 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -10.21 | 340.90 | -31.31 | 113.90 | 0.5616 | 663.0 | 537.7 | |
| 0.00 | 0.69 | 0.00 | 0.42 | -10.50 | 340.37 | -31.84 | 114.03 | 0.5702 | 136.0 | 195.5 | |
| 0.00 | 1.03 | 0.00 | 0.63 | -11.34 | 339.80 | -32.41 | 115.02 | 0.5822 | 633.0 | 557.8 | |
| 0.00 | 0.95 | 0.00 | 0.57 | -6.97 | 339.72 | -32.49 | 107.75 | 0.5620 | 691.0 | 517.0 | |
| 0.00 | 0.69 | 0.00 | 0.44 | -10.71 | 335.88 | -36.33 | 111.76 | 0.6290 | -711.0 | -573.0 | |
| 0.00 | 0.78 | 0.00 | 0.49 | -11.17 | 335.78 | -36.43 | 112.40 | 0.6325 | -573.0 | -536.8 | |
| 0.00 | 0.52 | 0.00 | 0.33 | -10.04 | 334.95 | -37.26 | 110.29 | 0.6378 | -642.0 | -583.5 | |
| 0.00 | 1.81 | 0.00 | 1.17 | -9.42 | 334.35 | -37.86 | 109.09 | 0.6430 | -761.0 | -590.1 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -10.79 | 333.62 | -38.59 | 110.76 | 0.6576 | -451.0 | -371.2 | |
| 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. | |