| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.64 | 0.00 | 13.32 | -4.98 | 139.20 | -30.68 | 110.07 | 0.5434 | -748.2 | -609.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.71 | -4.23 | 140.82 | -29.06 | 109.83 | 0.5170 | -736.0 | -581.7 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -4.41 | 140.22 | -29.66 | 109.76 | 0.5263 | -937.0 | -796.9 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -4.14 | 139.71 | -30.17 | 108.94 | 0.5320 | -980.0 | -868.7 | |
| 0.00 | 1.06 | 0.00 | 0.62 | -4.45 | 139.66 | -30.22 | 109.46 | 0.5343 | -821.0 | -677.4 | |
| 0.00 | 1.41 | 0.00 | 0.82 | -3.75 | 139.62 | -30.26 | 108.19 | 0.5313 | -871.0 | -638.0 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -4.98 | 139.46 | -30.42 | 110.26 | 0.5398 | -707.0 | -565.9 | |
| 0.00 | 0.62 | 0.00 | 0.36 | -4.87 | 139.29 | -30.59 | 109.95 | 0.5415 | -618.0 | -531.6 | |
| 0.00 | 1.94 | 0.00 | 1.15 | -6.32 | 139.17 | -30.71 | 112.35 | 0.5510 | -845.0 | -723.5 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -3.99 | 139.16 | -30.72 | 108.33 | 0.5390 | -794.0 | -575.1 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -6.52 | 138.91 | -30.97 | 112.51 | 0.5556 | -696.0 | -573.2 | |
| 0.00 | 1.59 | 0.00 | 0.94 | -5.93 | 138.91 | -30.97 | 111.53 | 0.5523 | -859.0 | -709.8 | |
| 0.00 | 1.76 | 0.00 | 1.04 | -5.47 | 138.91 | -30.97 | 110.74 | 0.5499 | -828.0 | -673.8 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -4.12 | 138.98 | -30.90 | 108.46 | 0.5421 | -793.0 | -614.5 | |
| 0.00 | 0.70 | 0.00 | 0.42 | -6.16 | 138.76 | -31.12 | 111.80 | 0.5556 | -559.0 | -434.0 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -4.56 | 138.82 | -31.06 | 109.12 | 0.5465 | -419.0 | -315.2 | |
| 0.00 | 2.82 | 0.00 | 1.66 | -4.16 | 138.76 | -31.12 | 108.40 | 0.5453 | -643.0 | -554.2 | |
| 0.00 | 1.41 | 0.00 | 0.84 | -6.66 | 138.55 | -31.33 | 112.50 | 0.5612 | -613.0 | -524.8 | |
| 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. | |