| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.88 | 91.18 | 22.42 | 97.79 | 17.29 | 355.03 | 62.15 | 287.65 | 0.8877 | -364.4 | -168.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.99 | 49.86 | 10.88 | 54.49 | 16.86 | 355.65 | 62.77 | 287.12 | 0.8923 | -545.1 | -25.6 | |
| 2.27 | -1.00 | 2.43 | -1.00 | 17.05 | 355.13 | 62.25 | 287.37 | 0.8885 | -609.6 | 999999 | |
| 1.73 | 3.18 | 1.83 | 3.37 | 16.62 | 354.82 | 61.94 | 286.92 | 0.8857 | -432.0 | -370.1 | |
| 1.63 | 4.63 | 1.76 | 4.94 | 17.59 | 355.17 | 62.30 | 287.97 | 0.8892 | -288.7 | -484.8 | |
| 1.45 | 2.36 | 1.55 | 2.53 | 17.34 | 355.03 | 62.15 | 287.71 | 0.8879 | -558.0 | -517.1 | |
| 0.00 | 1.45 | 0.00 | 1.54 | 17.12 | 354.90 | 62.02 | 287.48 | 0.8867 | -632.0 | -614.6 | |
| 0.00 | 2.63 | 0.00 | 2.77 | 16.98 | 354.61 | 61.74 | 287.35 | 0.8844 | -622.0 | -532.3 | |
| 0.00 | 1.00 | 0.00 | 1.04 | 16.55 | 354.30 | 61.43 | 286.89 | 0.8817 | -556.0 | -464.7 | |
| 0.00 | 1.00 | 0.00 | 1.05 | 17.36 | 354.63 | 61.75 | 287.77 | 0.8848 | -495.0 | -393.9 | |
| 2.18 | 17.71 | 2.35 | 19.06 | 18.84 | 355.06 | 62.18 | 289.39 | 0.8893 | 393.0 | -337.1 | |
| 1.63 | 4.00 | 1.62 | 3.95 | 16.42 | 352.60 | 59.73 | 286.91 | 0.8678 | -504.9 | -459.3 | |
| 0.00 | 1.18 | 0.00 | 1.08 | 16.13 | 349.67 | 56.79 | 286.91 | 0.8421 | 427.0 | 363.1 | |
| 0.00 | 1.09 | 0.00 | 0.99 | 16.84 | 349.46 | 56.59 | 287.77 | 0.8411 | 318.0 | 259.8 | |
| 0.00 | 1.09 | 0.00 | 0.98 | 16.45 | 349.05 | 56.18 | 287.37 | 0.8369 | 309.0 | 321.1 | |
| 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. | |