| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.74 | 63.43 | 19.60 | 50.69 | -20.17 | 140.01 | -50.93 | 111.68 | 0.7855 | 234.7 | 50.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.48 | 4.35 | 1.79 | 3.13 | -18.53 | 145.18 | -45.75 | 110.69 | 0.7284 | 851.6 | 672.8 | |
| 0.00 | 1.33 | 0.00 | 0.96 | -18.49 | 144.92 | -46.01 | 110.56 | 0.7311 | 608.0 | 571.1 | |
| 3.64 | 7.54 | 2.65 | 5.49 | -18.69 | 144.67 | -46.27 | 110.78 | 0.7344 | 677.2 | 471.0 | |
| 0.00 | 3.02 | 0.00 | 2.23 | -18.09 | 143.58 | -47.36 | 109.73 | 0.7452 | 651.0 | 499.1 | |
| 4.35 | 6.92 | 3.40 | 5.41 | -20.15 | 141.06 | -49.87 | 111.87 | 0.7758 | 718.2 | 492.9 | |
| 0.80 | 2.31 | 0.63 | 1.83 | -20.89 | 140.37 | -50.57 | 112.66 | 0.7842 | 606.7 | 503.1 | |
| 0.00 | 2.13 | 0.00 | 1.73 | -21.53 | 139.49 | -51.44 | 113.27 | 0.7941 | -138.0 | -124.1 | |
| 1.06 | 2.13 | 0.85 | 1.71 | -20.54 | 139.82 | -51.12 | 112.10 | 0.7890 | 453.8 | 340.8 | |
| 0.00 | 1.24 | 0.00 | 1.00 | -20.07 | 139.47 | -51.47 | 111.45 | 0.7917 | -662.0 | -607.7 | |
| 3.81 | 9.94 | 3.20 | 8.34 | -21.87 | 137.93 | -53.00 | 113.37 | 0.8096 | -698.3 | -506.0 | |
| 3.19 | 10.82 | 2.61 | 8.86 | -19.54 | 138.67 | -52.27 | 110.64 | 0.7987 | 549.2 | 357.8 | |
| 2.57 | -11.00 | 2.10 | -11.00 | -19.26 | 138.69 | -52.24 | 110.30 | 0.7980 | 663.9 | 999999 | |
| 2.84 | 4.70 | 2.37 | 3.93 | -20.11 | 137.81 | -53.12 | 111.20 | 0.8079 | 435.2 | 243.8 | |
| 0.00 | 0.53 | 0.00 | 0.46 | -22.12 | 136.58 | -54.36 | 113.42 | 0.8226 | -327.0 | -307.0 | |
| 0.00 | 1.24 | 0.00 | 1.07 | -21.97 | 136.61 | -54.32 | 113.24 | 0.8220 | -676.0 | -520.0 | |
| 0.00 | 3.90 | 0.00 | 3.39 | -21.47 | 136.38 | -54.55 | 112.60 | 0.8233 | -620.0 | -476.8 | |
| 0.00 | 1.33 | 0.00 | 1.15 | -20.92 | 136.63 | -54.30 | 111.97 | 0.8202 | -510.0 | -314.7 | |
| 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. | |