| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 190 | 1235 | 117 | 742 | 9.96 | 311.68 | 32.07 | 290.00 | 0.5537 | 314.7 | 135.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 119 | 684 | 76 | 434 | 9.51 | 317.14 | 37.53 | 285.93 | 0.6271 | 1323.7 | 566.0 | |
| 0 | 6 | 0 | 3 | 7.73 | 316.59 | 36.98 | 283.28 | 0.6148 | 740.0 | 543.1 | |
| 0 | 5 | 0 | 3 | 10.01 | 315.50 | 35.90 | 287.33 | 0.6071 | 804.0 | 890.6 | |
| 0 | 7 | 0 | 5 | 10.55 | 315.14 | 35.53 | 288.35 | 0.6043 | 912.0 | 808.4 | |
| 3 | 12 | 2 | 8 | 9.77 | 314.61 | 35.01 | 287.30 | 0.5944 | 914.8 | 831.4 | |
| 0 | 7 | 0 | 4 | 8.76 | 314.45 | 34.84 | 285.70 | 0.5888 | 783.0 | 679.8 | |
| 0 | 21 | 0 | 13 | 9.34 | 314.47 | 34.86 | 286.66 | 0.5910 | 1122.0 | 1035.2 | |
| 0 | 6 | 0 | 4 | 6.21 | 314.03 | 34.42 | 281.53 | 0.5758 | 886.0 | 657.3 | |
| 0 | 3 | 0 | 2 | 9.38 | 313.63 | 34.02 | 287.06 | 0.5796 | 808.0 | 673.7 | |
| 0 | 3 | 0 | 2 | 13.84 | 313.40 | 33.79 | 294.45 | 0.5955 | 776.0 | 653.0 | |
| 0 | 2 | 0 | 1 | 17.40 | 310.03 | 30.42 | 302.31 | 0.5740 | 553.0 | 546.5 | |
| 0 | 6 | 0 | 3 | 10.01 | 307.22 | 27.61 | 291.61 | 0.4929 | -785.0 | -618.1 | |
| 0 | 4 | 0 | 2 | 11.79 | 303.66 | 24.05 | 297.92 | 0.4534 | -480.0 | -357.1 | |
| 0 | 6 | 0 | 4 | 13.05 | 303.57 | 23.96 | 300.47 | 0.4609 | 652.0 | 473.4 | |
| 32 | 455 | 18 | 249 | 10.30 | 302.60 | 22.99 | 295.84 | 0.4287 | -1630.1 | -712.4 | |
| 7 | -15 | 4 | -15 | 10.50 | 301.77 | 22.16 | 297.05 | 0.4182 | -1755.5 | 999999 | |
| 23 | -15 | 13 | -15 | 11.31 | 301.66 | 22.05 | 298.92 | 0.4225 | -1735.8 | 999999 | |
| 6 | -15 | 4 | -15 | 10.81 | 301.54 | 21.93 | 297.96 | 0.4171 | -1970.8 | 999999 | |
| 0 | 5 | 0 | 3 | 9.79 | 301.42 | 21.81 | 295.84 | 0.4086 | -635.0 | -585.8 | |
| 0 | 3 | 0 | 2 | 14.26 | 301.43 | 21.82 | 305.13 | 0.4423 | -527.0 | -473.2 | |
| 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. | |