| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.57 | 43.86 | 5.62 | 23.31 | 7.12 | 208.83 | 21.34 | 272.33 | 0.3630 | -90.5 | -158.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.47 | 0.00 | 1.33 | 7.29 | 210.98 | 23.49 | 272.77 | 0.3975 | -762.0 | -615.3 | |
| 3.26 | 8.01 | 1.75 | 4.31 | 7.37 | 210.52 | 23.03 | 272.98 | 0.3902 | -1065.4 | -814.9 | |
| 0.00 | 0.97 | 0.00 | 0.52 | 7.87 | 210.12 | 22.63 | 274.29 | 0.3839 | -838.0 | -680.7 | |
| 0.79 | 3.87 | 0.42 | 2.07 | 7.01 | 209.75 | 22.26 | 272.04 | 0.3778 | -1047.3 | -798.4 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 7.95 | 209.67 | 22.18 | 274.53 | 0.3767 | -897.0 | -743.8 | |
| 0.00 | 1.23 | 0.00 | 0.66 | 6.37 | 209.36 | 21.87 | 270.29 | 0.3718 | -863.0 | -706.1 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 6.77 | 209.21 | 21.73 | 271.35 | 0.3693 | -124.0 | -31.0 | |
| 0.00 | 2.38 | 0.00 | 1.26 | 6.06 | 208.92 | 21.43 | 269.39 | 0.3650 | -855.0 | -818.7 | |
| 5.11 | 11.89 | 2.71 | 6.30 | 6.77 | 208.37 | 20.88 | 271.32 | 0.3556 | 802.8 | -10.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 7.47 | 207.63 | 20.14 | 273.31 | 0.3435 | 693.0 | 618.2 | |
| 0.00 | 1.50 | 0.00 | 0.79 | 7.31 | 207.04 | 19.55 | 272.86 | 0.3338 | 843.0 | 637.5 | |
| 0.00 | 0.62 | 0.00 | 0.32 | 7.01 | 207.03 | 19.54 | 271.96 | 0.3336 | 783.0 | 595.1 | |
| 1.41 | 5.64 | 0.74 | 2.96 | 7.70 | 206.93 | 19.44 | 274.06 | 0.3322 | 1114.0 | 856.1 | |
| 0.00 | 2.11 | 0.00 | 1.11 | 7.39 | 206.63 | 19.14 | 273.11 | 0.3271 | 868.0 | 675.5 | |
| 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. | |