| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.09 | 61.50 | 17.89 | 45.98 | -15.87 | 246.24 | -46.23 | 111.89 | 0.7504 | 110.4 | 66.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.17 | 5.61 | 1.56 | 4.04 | -15.91 | 248.48 | -43.99 | 112.73 | 0.7265 | 842.4 | 654.7 | |
| 0.00 | 2.99 | 0.00 | 2.15 | -15.75 | 248.30 | -44.17 | 112.45 | 0.7279 | 801.0 | 650.5 | |
| 2.90 | 3.62 | 2.09 | 2.61 | -15.50 | 248.06 | -44.41 | 112.03 | 0.7298 | 801.4 | 599.2 | |
| 7.52 | 9.42 | 5.47 | 6.85 | -15.70 | 247.65 | -44.82 | 112.14 | 0.7349 | 627.7 | 484.1 | |
| 1.09 | 4.98 | 0.79 | 3.62 | -15.38 | 247.65 | -44.82 | 111.72 | 0.7339 | 657.7 | 541.6 | |
| 0.91 | 3.53 | 0.66 | 2.59 | -15.98 | 247.39 | -45.08 | 112.42 | 0.7387 | 435.2 | 260.5 | |
| 2.26 | 4.80 | 1.66 | 3.52 | -15.29 | 247.18 | -45.29 | 111.44 | 0.7388 | 523.4 | 425.6 | |
| 0.00 | 1.63 | 0.00 | 1.20 | -15.16 | 246.81 | -45.66 | 111.15 | 0.7425 | 464.0 | 340.4 | |
| 0.00 | 0.91 | 0.00 | 0.67 | -15.20 | 246.39 | -46.08 | 111.05 | 0.7472 | 453.0 | 411.2 | |
| 0.00 | 1.27 | 0.00 | 0.94 | -14.50 | 246.35 | -46.12 | 110.14 | 0.7455 | 558.0 | 459.9 | |
| 0.00 | 1.81 | 0.00 | 1.38 | -15.36 | 245.18 | -47.29 | 110.88 | 0.7606 | -659.0 | -538.7 | |
| 7.24 | 14.22 | 5.66 | 11.12 | -16.45 | 244.08 | -48.39 | 111.91 | 0.7751 | -778.6 | -595.3 | |
| 0.00 | 1.54 | 0.00 | 1.20 | -16.32 | 243.93 | -48.54 | 111.70 | 0.7763 | -528.0 | -519.4 | |
| 0.00 | 1.36 | 0.00 | 1.07 | -16.39 | 243.57 | -48.90 | 111.67 | 0.7802 | -472.0 | -421.1 | |
| 0.00 | 1.54 | 0.00 | 1.22 | -16.52 | 243.23 | -49.24 | 111.73 | 0.7839 | -477.0 | -277.9 | |
| 0.00 | 1.18 | 0.00 | 0.94 | -16.62 | 243.20 | -49.27 | 111.84 | 0.7845 | -383.0 | -363.9 | |
| 0.00 | 1.09 | 0.00 | 0.86 | -15.85 | 243.07 | -49.40 | 110.86 | 0.7838 | -368.0 | -362.5 | |
| 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. | |