| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.96 | 386.27 | 33.83 | 214.11 | 11.90 | 274.91 | 20.13 | 311.29 | 0.4501 | -846.5 | -334.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.96 | 360.17 | 33.83 | 199.93 | 11.77 | 275.31 | 20.53 | 310.42 | 0.4529 | -1445.2 | -418.2 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 13.95 | 272.05 | 17.28 | 318.88 | 0.4402 | -603.0 | -509.8 | |
| 0.00 | 1.95 | 0.00 | 1.06 | 12.80 | 270.58 | 15.81 | 319.58 | 0.4114 | 805.0 | 673.8 | |
| 0.00 | 5.31 | 0.00 | 2.88 | 12.89 | 270.40 | 15.62 | 320.06 | 0.4106 | 860.0 | 726.5 | |
| 0.00 | 2.65 | 0.00 | 1.44 | 13.10 | 270.06 | 15.28 | 321.01 | 0.4098 | 1088.0 | 918.2 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 13.89 | 269.73 | 14.95 | 322.83 | 0.4163 | 628.0 | 521.6 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 14.35 | 269.18 | 14.41 | 324.52 | 0.4170 | 682.0 | 520.6 | |
| 0.00 | 1.50 | 0.00 | 0.82 | 14.38 | 269.02 | 14.25 | 324.86 | 0.4159 | 914.0 | 793.8 | |
| 0.00 | 3.10 | 0.00 | 1.69 | 14.79 | 268.63 | 13.86 | 326.17 | 0.4177 | 840.0 | 689.2 | |
| 0.00 | 0.97 | 0.00 | 0.54 | 17.41 | 268.50 | 13.72 | 329.74 | 0.4512 | 712.0 | 534.4 | |
| 0.00 | 3.01 | 0.00 | 1.63 | 14.53 | 268.26 | 13.49 | 326.52 | 0.4110 | 925.0 | 847.4 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 13.65 | 267.54 | 12.77 | 326.72 | 0.3930 | 789.0 | 611.0 | |
| 0.00 | 2.03 | 0.00 | 1.10 | 13.74 | 267.32 | 12.55 | 327.30 | 0.3923 | 762.0 | 597.2 | |
| 0.00 | 1.24 | 0.00 | 0.66 | 11.84 | 266.00 | 11.23 | 327.39 | 0.3551 | 848.0 | 562.6 | |
| 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. | |