| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.78 | 362.87 | 52.24 | 275.87 | -8.92 | 320.01 | -47.17 | 107.18 | 0.7596 | 557.8 | 251.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.36 | 0.00 | 1.71 | -8.35 | 322.33 | -44.84 | 107.26 | 0.7329 | 381.0 | 258.1 | |
| 2.45 | 332.10 | 1.81 | 247.73 | -8.28 | 321.22 | -45.96 | 106.75 | 0.7452 | 982.6 | 300.0 | |
| 24.22 | -2.00 | 18.08 | -2.00 | -9.19 | 320.98 | -46.19 | 107.84 | 0.7507 | 925.2 | 999999 | |
| 21.16 | -2.00 | 15.76 | -2.00 | -8.60 | 320.99 | -46.18 | 107.09 | 0.7487 | 951.9 | 999999 | |
| 10.76 | -2.00 | 8.08 | -2.00 | -8.91 | 320.64 | -46.54 | 107.35 | 0.7536 | 651.2 | 999999 | |
| 1.05 | -2.00 | 0.79 | -2.00 | -8.74 | 320.40 | -46.78 | 107.05 | 0.7557 | 137.6 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.69 | -7.65 | 317.90 | -49.28 | 104.84 | 0.7794 | 365.0 | 228.7 | |
| 0.00 | 1.49 | 0.00 | 1.27 | -9.83 | 314.83 | -52.35 | 106.56 | 0.8161 | -527.0 | -480.8 | |
| 0.00 | 3.76 | 0.00 | 3.36 | -9.87 | 312.93 | -54.25 | 106.04 | 0.8341 | -653.0 | -544.7 | |
| 0.00 | 0.61 | 0.00 | 0.54 | -8.22 | 313.14 | -54.04 | 104.16 | 0.8283 | -543.0 | -506.0 | |
| 0.00 | 0.26 | 0.00 | 0.24 | -9.98 | 312.43 | -54.75 | 106.02 | 0.8389 | -402.0 | -379.3 | |
| 0.00 | 0.61 | 0.00 | 0.58 | -11.24 | 311.11 | -56.07 | 107.09 | 0.8535 | -147.0 | -194.9 | |
| 5.95 | 16.61 | 5.61 | 15.70 | -8.96 | 310.57 | -56.61 | 104.35 | 0.8534 | -614.5 | -198.0 | |
| 2.19 | 4.20 | 2.11 | 4.05 | -9.90 | 310.04 | -57.13 | 105.29 | 0.8598 | -409.5 | -271.2 | |
| 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. | |