| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.96 | 0.00 | 14.07 | -17.44 | 327.91 | -30.83 | 113.13 | 0.5318 | 295.5 | 343.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.82 | 0.00 | 1.54 | -13.58 | 334.17 | -24.57 | 108.94 | 0.4292 | 871.0 | 679.7 | |
| 0.00 | 2.20 | 0.00 | 1.22 | -14.69 | 333.04 | -25.70 | 110.71 | 0.4503 | 667.0 | 556.4 | |
| 0.00 | 1.41 | 0.00 | 0.79 | -15.90 | 332.15 | -26.59 | 112.70 | 0.4686 | 733.0 | 603.6 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -13.69 | 332.44 | -26.30 | 108.24 | 0.4551 | -567.0 | -416.8 | |
| 0.00 | 1.59 | 0.00 | 0.89 | -17.26 | 331.84 | -26.90 | 115.23 | 0.4797 | 635.0 | 494.8 | |
| 0.00 | 1.59 | 0.00 | 0.92 | -18.03 | 329.38 | -29.36 | 115.14 | 0.5171 | 644.0 | 552.9 | |
| 0.00 | 1.59 | 0.00 | 0.91 | -15.73 | 328.80 | -29.93 | 110.55 | 0.5150 | 567.0 | 489.9 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -24.17 | 326.64 | -32.10 | 123.77 | 0.5854 | 738.0 | 650.0 | |
| 0.00 | 1.85 | 0.00 | 1.07 | -14.37 | 328.44 | -30.30 | 107.81 | 0.5153 | 658.0 | 507.9 | |
| 0.00 | 2.20 | 0.00 | 1.30 | -18.85 | 327.45 | -31.29 | 115.51 | 0.5467 | 705.0 | 553.4 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -19.05 | 327.19 | -31.55 | 115.72 | 0.5511 | 707.0 | 603.6 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -16.76 | 327.53 | -31.21 | 111.85 | 0.5366 | 617.0 | 522.1 | |
| 0.00 | 1.32 | 0.00 | 0.78 | -18.89 | 327.07 | -31.67 | 115.38 | 0.5519 | 712.0 | 625.1 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -21.12 | 319.61 | -39.13 | 115.49 | 0.6544 | -684.0 | -529.8 | |
| 0.00 | 1.23 | 0.00 | 0.80 | -18.48 | 319.36 | -39.38 | 111.46 | 0.6488 | -718.0 | -589.9 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -22.28 | 316.26 | -42.48 | 115.92 | 0.6972 | -691.0 | -604.0 | |
| 0.00 | 0.88 | 0.00 | 0.61 | -22.91 | 315.83 | -42.91 | 116.65 | 0.7040 | -571.0 | -498.1 | |
| 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. | |