| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.91 | 47.20 | 26.49 | 78.94 | 18.94 | 315.37 | 72.28 | 289.36 | 0.9552 | -198.4 | -87.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.14 | 2.74 | 4.07 | 5.22 | 17.65 | 317.83 | 74.74 | 287.83 | 0.9669 | -276.7 | -53.6 | |
| 7.37 | 13.62 | 14.45 | 26.83 | 18.86 | 318.23 | 75.14 | 289.06 | 0.9689 | -379.7 | -113.5 | |
| 0.00 | 0.86 | 0.00 | 1.50 | 18.44 | 316.33 | 73.24 | 288.74 | 0.9605 | -533.0 | -498.4 | |
| 0.00 | 4.97 | 0.00 | 8.73 | 19.13 | 316.34 | 73.25 | 289.45 | 0.9608 | -494.0 | -428.5 | |
| 0.00 | 1.03 | 0.00 | 1.59 | 17.63 | 313.96 | 70.87 | 288.06 | 0.9485 | 313.0 | 198.3 | |
| 0.00 | 1.54 | 0.00 | 2.58 | 19.31 | 315.47 | 72.38 | 289.70 | 0.9568 | -410.0 | -297.0 | |
| 1.71 | 2.06 | 2.69 | 3.23 | 19.31 | 314.15 | 71.06 | 289.81 | 0.9502 | -332.8 | -347.8 | |
| 1.46 | 8.74 | 2.10 | 12.71 | 18.91 | 312.45 | 69.36 | 289.55 | 0.9409 | 287.4 | -42.8 | |
| 0.00 | 1.11 | 0.00 | 1.68 | 20.02 | 313.35 | 70.26 | 290.63 | 0.9464 | -428.0 | -326.8 | |
| 0.00 | 1.37 | 0.00 | 1.89 | 18.07 | 311.45 | 68.36 | 288.74 | 0.9347 | 46.0 | 65.0 | |
| 2.23 | 7.54 | 3.18 | 10.78 | 19.64 | 312.06 | 68.97 | 290.36 | 0.9392 | 379.8 | 309.4 | |
| 0.00 | 0.51 | 0.00 | 0.70 | 18.64 | 311.00 | 67.90 | 289.39 | 0.9324 | 14.0 | 73.5 | |
| 0.00 | 1.11 | 0.00 | 1.50 | 19.49 | 310.72 | 67.63 | 290.33 | 0.9313 | 346.0 | 315.1 | |
| 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. | |