| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.56 | 192.31 | 57.05 | 455.82 | 15.49 | 60.14 | -79.06 | 75.50 | 0.9761 | -269.7 | -30.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.46 | 105.03 | 16.30 | 186.03 | 15.91 | 64.78 | -74.43 | 75.34 | 0.9588 | -649.5 | -97.0 | |
| 1.44 | -1.00 | 2.55 | -1.00 | 15.75 | 64.21 | -74.99 | 75.48 | 0.9615 | 166.8 | 999999 | |
| 4.86 | -1.00 | 8.89 | -1.00 | 15.51 | 63.72 | -75.48 | 75.72 | 0.9638 | 250.9 | 999999 | |
| 2.52 | -1.00 | 4.56 | -1.00 | 15.25 | 63.99 | -75.21 | 75.99 | 0.9626 | -194.8 | 999999 | |
| 3.15 | 24.86 | 7.15 | 58.15 | 16.50 | 60.42 | -78.78 | 74.52 | 0.9769 | -202.4 | 101.9 | |
| 0.00 | 1.80 | 0.00 | 3.83 | 15.06 | 61.46 | -77.75 | 76.05 | 0.9733 | 368.0 | 353.6 | |
| 0.00 | 10.36 | 0.00 | 37.67 | 18.19 | 55.34 | -83.86 | 72.48 | 0.9912 | 309.0 | 215.1 | |
| 0.00 | 2.52 | 0.00 | 5.98 | 15.36 | 59.92 | -79.29 | 75.65 | 0.9789 | 495.0 | 487.1 | |
| 0.00 | 0.99 | 0.00 | 2.33 | 15.21 | 59.97 | -79.24 | 75.81 | 0.9788 | 569.0 | 526.2 | |
| 0.00 | 1.08 | 0.00 | 2.76 | 15.58 | 59.03 | -80.17 | 75.37 | 0.9818 | 446.0 | 432.1 | |
| 0.00 | 1.44 | 0.00 | 3.62 | 15.15 | 59.16 | -80.05 | 75.82 | 0.9815 | 442.0 | 436.8 | |
| 0.00 | 0.72 | 0.00 | 1.88 | 15.29 | 58.74 | -80.47 | 75.64 | 0.9828 | 424.0 | 383.8 | |
| 5.13 | 43.51 | 17.60 | 153.57 | 14.24 | 56.18 | -83.03 | 76.51 | 0.9900 | -571.6 | -144.4 | |
| 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. | |