| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.93 | 222.35 | 59.08 | 388.76 | 20.39 | 186.94 | 70.47 | 292.81 | 0.9576 | 111.2 | 34.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.87 | 48.12 | 4.78 | 120.43 | 20.05 | 192.87 | 76.40 | 291.42 | 0.9817 | 389.4 | -32.0 | |
| 4.28 | -1.00 | 10.37 | -1.00 | 20.00 | 192.25 | 75.78 | 291.46 | 0.9797 | -497.5 | 999999 | |
| 0.00 | 2.41 | 0.00 | 4.39 | 19.43 | 188.06 | 71.59 | 291.58 | 0.9634 | -444.0 | -330.7 | |
| 1.07 | 4.19 | 1.83 | 7.14 | 19.61 | 186.95 | 70.48 | 291.96 | 0.9586 | 239.9 | 68.6 | |
| 0.00 | 2.32 | 0.00 | 3.99 | 20.13 | 186.90 | 70.43 | 292.50 | 0.9588 | -169.0 | -100.0 | |
| 2.23 | 153.81 | 3.52 | 235.02 | 20.20 | 185.20 | 68.73 | 292.91 | 0.9508 | 307.3 | 79.4 | |
| 6.33 | -6.00 | 10.09 | -6.00 | 20.57 | 185.28 | 68.81 | 293.27 | 0.9516 | -502.5 | 999999 | |
| 1.78 | -6.00 | 2.70 | -6.00 | 20.47 | 184.30 | 67.83 | 293.37 | 0.9465 | -194.2 | 999999 | |
| 11.67 | -6.00 | 17.44 | -6.00 | 20.38 | 183.96 | 67.49 | 293.35 | 0.9447 | 504.6 | 999999 | |
| 0.00 | 0.27 | 0.00 | 0.43 | 21.86 | 184.96 | 68.49 | 294.67 | 0.9515 | -321.0 | -337.7 | |
| 1.60 | -6.00 | 2.41 | -6.00 | 20.93 | 183.96 | 67.49 | 293.92 | 0.9454 | 351.9 | 999999 | |
| 4.10 | -6.00 | 5.94 | -6.00 | 20.75 | 183.21 | 66.73 | 293.90 | 0.9411 | 836.0 | 999999 | |
| 0.00 | 9.27 | 0.00 | 14.44 | 22.09 | 184.49 | 68.01 | 295.01 | 0.9494 | -61.0 | -21.1 | |
| 0.00 | 1.07 | 0.00 | 1.62 | 21.76 | 183.98 | 67.51 | 294.77 | 0.9465 | 507.0 | 439.8 | |
| 0.00 | 0.89 | 0.00 | 1.30 | 21.73 | 183.11 | 66.63 | 294.94 | 0.9419 | 482.0 | 415.6 | |
| 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. | |