| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.78 | 235.19 | 31.99 | 129.87 | -13.20 | 121.27 | -17.29 | 139.08 | 0.4431 | 452.5 | 278.9 | |
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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 | 0.67 | -12.98 | 123.46 | -15.10 | 142.46 | 0.4183 | 695.0 | 626.5 | |
| 21.81 | 197.93 | 11.97 | 108.81 | -13.15 | 122.14 | -16.42 | 140.36 | 0.4334 | 1208.5 | 357.6 | |
| 12.75 | -2.00 | 7.00 | -2.00 | -12.93 | 121.90 | -16.66 | 139.63 | 0.4333 | 1107.9 | 999999 | |
| 6.16 | -2.00 | 3.40 | -2.00 | -13.42 | 121.57 | -16.99 | 139.82 | 0.4424 | 837.0 | 999999 | |
| 2.99 | -2.00 | 1.65 | -2.00 | -13.52 | 121.34 | -17.22 | 139.59 | 0.4459 | 664.9 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -13.63 | 120.97 | -17.59 | 139.16 | 0.4509 | 639.0 | 554.6 | |
| 0.44 | 2.02 | 0.24 | 1.12 | -13.51 | 120.82 | -17.74 | 138.73 | 0.4510 | 791.6 | 650.4 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -13.27 | 120.29 | -18.27 | 137.53 | 0.4539 | 557.0 | 517.3 | |
| 0.44 | 2.37 | 0.25 | 1.33 | -13.28 | 119.38 | -19.18 | 136.15 | 0.4635 | 537.2 | 489.2 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -12.83 | 118.53 | -20.03 | 134.22 | 0.4679 | 765.0 | 607.6 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -15.48 | 117.92 | -20.65 | 137.28 | 0.5029 | -738.0 | -607.5 | |
| 0.79 | 7.03 | 0.45 | 3.98 | -13.22 | 117.51 | -21.05 | 133.41 | 0.4833 | -976.2 | -727.9 | |
| 2.99 | -12.00 | 1.69 | -12.00 | -13.48 | 117.42 | -21.14 | 133.68 | 0.4870 | -914.0 | 999999 | |
| 0.00 | 2.46 | 0.00 | 1.41 | -14.80 | 117.29 | -21.27 | 135.46 | 0.5021 | -743.0 | -570.1 | |
| 0.00 | 1.58 | 0.00 | 0.89 | -12.76 | 117.26 | -21.31 | 132.34 | 0.4814 | -805.0 | -577.7 | |
| 9.41 | 15.21 | 5.34 | 8.64 | -13.22 | 116.85 | -21.71 | 132.52 | 0.4906 | -985.7 | -658.2 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -14.32 | 115.16 | -23.40 | 132.04 | 0.5202 | -512.0 | -441.1 | |
| 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. | |