| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.51 | 30.93 | 1.79 | 15.81 | 14.16 | 91.63 | -10.08 | 134.71 | 0.2215 | -170.3 | -37.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.61 | 9.39 | 101.75 | 0.04 | 359.33 | 0.0525 | -913.0 | -753.3 | |
| 0.00 | 1.05 | 0.00 | 0.52 | 10.59 | 101.66 | -0.05 | 0.73 | 0.0736 | -788.0 | -589.0 | |
| 0.00 | 0.97 | 0.00 | 0.48 | 9.00 | 101.63 | -0.09 | 1.87 | 0.0457 | -939.0 | -706.1 | |
| 0.00 | 2.02 | 0.00 | 1.00 | 10.05 | 99.20 | -2.52 | 34.14 | 0.0775 | -916.0 | -731.5 | |
| 0.00 | 1.05 | 0.00 | 0.52 | 10.77 | 98.82 | -2.89 | 32.96 | 0.0915 | -753.0 | -609.9 | |
| 0.00 | 2.90 | 0.00 | 1.44 | 10.64 | 97.76 | -3.96 | 42.39 | 0.1011 | -647.0 | -611.2 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 10.64 | 97.11 | -4.60 | 46.68 | 0.1089 | -811.0 | -610.2 | |
| 0.00 | 1.41 | 0.00 | 0.70 | 11.86 | 96.64 | -5.08 | 42.13 | 0.1298 | -887.0 | -630.9 | |
| 0.00 | 1.14 | 0.00 | 0.57 | 12.01 | 93.58 | -8.14 | 54.43 | 0.1710 | -921.0 | -716.8 | |
| 0.00 | 0.97 | 0.00 | 0.49 | 12.21 | 92.86 | -8.85 | 55.69 | 0.1830 | -676.0 | -529.0 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 19.10 | 90.37 | -11.34 | 39.94 | 0.2908 | 791.0 | 675.1 | |
| 3.51 | 7.47 | 1.79 | 3.81 | 13.47 | 89.46 | -12.25 | 58.64 | 0.2428 | 1227.5 | 894.4 | |
| 0.00 | 1.41 | 0.00 | 0.73 | 18.97 | 88.79 | -12.92 | 43.82 | 0.3068 | 827.0 | 677.1 | |
| 0.00 | 1.58 | 0.00 | 0.82 | 17.23 | 86.62 | -15.09 | 52.37 | 0.3154 | 825.0 | 616.3 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 24.99 | 84.25 | -17.47 | 40.06 | 0.4246 | 902.0 | 723.1 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 11.36 | 82.12 | -19.60 | 74.21 | 0.3432 | -763.0 | -482.3 | |
| 0.00 | 2.46 | 0.00 | 1.37 | 22.37 | 78.77 | -22.95 | 51.83 | 0.4606 | 443.0 | 334.0 | |
| 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. | |