| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.15 | 131.95 | 28.90 | 112.03 | 7.03 | 210.80 | 54.67 | 273.90 | 0.8131 | -70.9 | -40.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.36 | 75.44 | 7.45 | 66.86 | 7.38 | 212.82 | 56.69 | 274.47 | 0.8334 | -721.4 | -281.1 | |
| 10.39 | -1.00 | 9.16 | -1.00 | 7.24 | 212.41 | 56.27 | 274.27 | 0.8295 | -850.3 | 999999 | |
| 0.00 | 1.58 | 0.00 | 1.35 | 7.16 | 211.05 | 54.91 | 274.08 | 0.8161 | -356.0 | -465.0 | |
| 0.00 | 0.26 | 0.00 | 0.23 | 7.31 | 211.07 | 54.94 | 274.27 | 0.8163 | -329.0 | -285.0 | |
| 0.00 | 1.06 | 0.00 | 0.89 | 6.27 | 210.58 | 54.44 | 272.95 | 0.8120 | -282.0 | -365.2 | |
| 0.00 | 0.88 | 0.00 | 0.72 | 6.72 | 209.01 | 52.87 | 273.39 | 0.7955 | 189.0 | 130.7 | |
| 0.00 | 0.97 | 0.00 | 0.78 | 6.88 | 208.84 | 52.70 | 273.59 | 0.7935 | 362.0 | 332.2 | |
| 0.00 | 3.52 | 0.00 | 2.85 | 7.04 | 208.76 | 52.62 | 273.79 | 0.7927 | 561.0 | 352.7 | |
| 8.36 | 20.07 | 6.72 | 16.15 | 6.40 | 208.46 | 52.33 | 272.96 | 0.7899 | 590.8 | 220.4 | |
| 0.00 | 1.32 | 0.00 | 1.05 | 6.98 | 208.15 | 52.02 | 273.66 | 0.7862 | 290.0 | 298.4 | |
| 0.70 | 20.25 | 0.56 | 16.03 | 6.38 | 208.01 | 51.88 | 272.90 | 0.7851 | 500.5 | 580.1 | |
| 0.00 | 1.23 | 0.00 | 0.98 | 6.13 | 207.78 | 51.65 | 272.56 | 0.7827 | 400.0 | 420.4 | |
| 3.26 | -11.00 | 2.58 | -11.00 | 6.71 | 207.72 | 51.58 | 273.30 | 0.7817 | 831.1 | 999999 | |
| 3.08 | -11.00 | 2.43 | -11.00 | 6.55 | 207.55 | 51.41 | 273.08 | 0.7799 | 749.4 | 999999 | |
| 0.00 | 2.99 | 0.00 | 2.32 | 7.16 | 206.82 | 50.68 | 273.81 | 0.7716 | 511.0 | 386.8 | |
| 0.00 | 0.97 | 0.00 | 0.75 | 6.53 | 206.68 | 50.54 | 273.00 | 0.7704 | 336.0 | 376.1 | |
| 0.00 | 1.41 | 0.00 | 1.07 | 7.30 | 205.89 | 49.75 | 273.95 | 0.7612 | 438.0 | 386.2 | |
| 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. | |