| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.87 | 113.60 | 43.95 | 148.01 | 8.55 | 102.39 | 66.53 | 281.15 | 0.9238 | 214.2 | 125.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.78 | 0.00 | 3.58 | 6.64 | 110.96 | 75.10 | 277.97 | 0.9704 | 395.0 | 215.6 | |
| 0.00 | 1.36 | 0.00 | 2.66 | 6.14 | 110.62 | 74.77 | 277.49 | 0.9687 | -193.0 | -147.2 | |
| 1.36 | 10.71 | 2.64 | 20.91 | 6.37 | 110.49 | 74.63 | 277.74 | 0.9683 | -335.4 | -150.2 | |
| 3.91 | -3.00 | 7.64 | -3.00 | 6.81 | 110.46 | 74.60 | 278.20 | 0.9683 | 49.3 | 999999 | |
| 0.00 | 0.76 | 0.00 | 1.35 | 5.60 | 109.01 | 73.15 | 277.11 | 0.9612 | -286.0 | -273.2 | |
| 3.14 | 4.93 | 4.70 | 7.37 | 6.98 | 105.77 | 69.91 | 278.95 | 0.9451 | -330.2 | -171.6 | |
| 0.00 | 0.51 | 0.00 | 0.84 | 10.30 | 107.14 | 71.29 | 282.23 | 0.9549 | 49.0 | 81.3 | |
| 0.00 | 0.68 | 0.00 | 0.99 | 7.20 | 105.07 | 69.21 | 279.27 | 0.9413 | -254.0 | -284.5 | |
| 0.00 | 1.53 | 0.00 | 2.12 | 6.72 | 104.16 | 68.31 | 278.88 | 0.9355 | -449.0 | -390.8 | |
| 1.27 | 2.04 | 1.73 | 2.76 | 8.53 | 103.41 | 67.55 | 280.91 | 0.9324 | 142.1 | 43.7 | |
| 0.00 | 2.04 | 0.00 | 2.53 | 9.25 | 101.18 | 65.32 | 282.03 | 0.9187 | 138.0 | 1.3 | |
| 0.00 | 1.10 | 0.00 | 1.33 | 8.07 | 100.64 | 64.79 | 280.84 | 0.9138 | 344.0 | 290.4 | |
| 3.40 | 63.22 | 4.11 | 75.22 | 9.47 | 100.48 | 64.62 | 282.39 | 0.9142 | 167.8 | 164.1 | |
| 3.48 | 8.16 | 4.09 | 9.58 | 7.96 | 99.91 | 64.06 | 280.83 | 0.9085 | 144.9 | 124.3 | |
| 0.68 | 1.61 | 0.80 | 1.91 | 8.26 | 100.00 | 64.15 | 281.15 | 0.9095 | 514.8 | 465.8 | |
| 5.10 | -13.00 | 6.07 | -13.00 | 9.32 | 100.07 | 64.22 | 282.29 | 0.9112 | 480.5 | 999999 | |
| 6.03 | -13.00 | 7.07 | -13.00 | 9.48 | 99.64 | 63.79 | 282.53 | 0.9083 | 742.9 | 999999 | |
| 4.50 | 13.17 | 5.10 | 14.86 | 9.29 | 98.71 | 62.85 | 282.50 | 0.9013 | 653.8 | 508.1 | |
| 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. | |