| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.58 | 458.21 | 80.09 | 444.15 | -17.63 | 105.91 | 54.61 | 244.69 | 0.8598 | 40.6 | -25.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.98 | 232.53 | 43.26 | 245.54 | -17.00 | 109.24 | 57.94 | 246.65 | 0.8847 | 720.4 | 168.0 | |
| 0.00 | 1.08 | 0.00 | 1.09 | -17.01 | 107.77 | 56.47 | 246.14 | 0.8736 | 554.0 | 488.6 | |
| 0.00 | 0.81 | 0.00 | 0.78 | -16.53 | 106.25 | 54.95 | 246.14 | 0.8602 | 544.0 | 420.3 | |
| 2.07 | 3.15 | 2.02 | 3.07 | -17.23 | 106.39 | 55.09 | 245.42 | 0.8633 | 509.3 | 376.2 | |
| 0.00 | 1.26 | 0.00 | 1.22 | -17.49 | 106.01 | 54.70 | 244.99 | 0.8610 | 466.0 | 390.5 | |
| 0.00 | 0.63 | 0.00 | 0.61 | -17.85 | 105.67 | 54.37 | 244.47 | 0.8594 | 402.0 | 312.7 | |
| 0.00 | 1.35 | 0.00 | 1.26 | -18.03 | 104.50 | 53.20 | 243.83 | 0.8504 | -237.0 | -229.1 | |
| 0.00 | 0.90 | 0.00 | 0.86 | -19.68 | 104.77 | 53.47 | 242.12 | 0.8580 | -213.0 | -159.4 | |
| 0.00 | 1.53 | 0.00 | 1.44 | -19.37 | 104.30 | 53.00 | 242.28 | 0.8532 | -536.0 | -375.1 | |
| 2.79 | 5.04 | 2.64 | 4.77 | -19.69 | 104.24 | 52.94 | 241.89 | 0.8538 | -549.6 | -382.5 | |
| 0.00 | 0.36 | 0.00 | 0.34 | -20.11 | 104.06 | 52.76 | 241.37 | 0.8538 | -381.0 | -322.5 | |
| 1.17 | 209.57 | 1.03 | 183.17 | -17.80 | 102.16 | 50.86 | 243.13 | 0.8300 | -254.1 | -286.7 | |
| 18.46 | -12.00 | 16.26 | -12.00 | -18.64 | 101.64 | 50.34 | 241.96 | 0.8285 | -715.0 | 999999 | |
| 17.11 | -12.00 | 14.88 | -12.00 | -18.21 | 101.32 | 50.01 | 242.30 | 0.8241 | -1067.5 | 999999 | |
| 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. | |