| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.11 | 25.13 | 1.11 | 13.53 | 4.81 | 25.67 | -19.79 | 60.77 | 0.3870 | -175.3 | -329.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.35 | 0.00 | 0.19 | 6.94 | 28.91 | -16.55 | 51.34 | 0.3637 | -331.0 | -492.2 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 4.17 | 28.39 | -17.07 | 58.61 | 0.3444 | -819.0 | -606.7 | |
| 2.11 | 7.99 | 1.11 | 4.21 | 3.72 | 28.31 | -17.15 | 59.88 | 0.3417 | -1184.6 | -818.0 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 3.96 | 28.24 | -17.22 | 59.36 | 0.3448 | -935.0 | -737.1 | |
| 0.00 | 3.43 | 0.00 | 1.81 | 4.09 | 28.14 | -17.32 | 59.20 | 0.3472 | -708.0 | -716.5 | |
| 0.00 | 2.37 | 0.00 | 1.24 | 1.29 | 28.18 | -17.28 | 66.54 | 0.3252 | -829.0 | -654.2 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 3.29 | 27.34 | -18.12 | 62.32 | 0.3522 | -653.0 | -517.4 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 3.19 | 26.80 | -18.66 | 63.27 | 0.3592 | -830.0 | -696.5 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 8.49 | 23.91 | -21.55 | 55.54 | 0.4425 | 767.0 | 566.0 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 8.67 | 23.47 | -21.99 | 55.76 | 0.4496 | 694.0 | 580.6 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 9.02 | 19.33 | -26.14 | 59.65 | 0.5062 | 524.0 | 367.2 | |
| 0.00 | 2.11 | 0.00 | 1.21 | 7.83 | 18.36 | -27.10 | 62.62 | 0.5103 | 693.0 | 496.0 | |
| 0.00 | 0.88 | 0.00 | 0.51 | 7.40 | 17.88 | -27.58 | 63.80 | 0.5138 | 615.0 | 477.0 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 6.22 | 17.54 | -27.92 | 66.17 | 0.5109 | 654.0 | 466.8 | |
| 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. | |