| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.31 | 0.00 | 13.56 | 16.48 | 24.63 | -8.46 | 21.44 | 0.3849 | 206.3 | 246.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.85 | 0.00 | 0.45 | 16.41 | 30.32 | -2.77 | 7.47 | 0.3584 | -760.0 | -599.7 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 16.16 | 29.92 | -3.17 | 8.64 | 0.3552 | -934.0 | -731.2 | |
| 0.00 | 0.76 | 0.00 | 0.41 | 16.33 | 28.41 | -4.68 | 12.53 | 0.3624 | -791.0 | -644.7 | |
| 0.00 | 1.10 | 0.00 | 0.59 | 16.36 | 28.20 | -4.90 | 13.07 | 0.3638 | -837.0 | -645.4 | |
| 0.00 | 2.21 | 0.00 | 1.17 | 16.21 | 27.55 | -5.54 | 14.83 | 0.3639 | -1123.0 | -966.4 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.21 | 27.31 | -5.79 | 15.45 | 0.3650 | -876.0 | -705.1 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 17.35 | 24.07 | -9.03 | 22.13 | 0.3993 | 846.0 | 535.0 | |
| 0.00 | 1.87 | 0.00 | 1.00 | 16.22 | 23.87 | -9.22 | 23.75 | 0.3838 | 968.0 | 907.1 | |
| 0.00 | 2.80 | 0.00 | 1.50 | 15.84 | 23.70 | -9.39 | 24.56 | 0.3794 | 803.0 | 720.2 | |
| 0.00 | 1.70 | 0.00 | 0.91 | 16.38 | 23.55 | -9.54 | 24.29 | 0.3883 | 669.0 | 515.7 | |
| 0.00 | 2.38 | 0.00 | 1.27 | 15.91 | 23.36 | -9.74 | 25.27 | 0.3828 | 774.0 | 695.7 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 17.02 | 22.80 | -10.29 | 25.23 | 0.4027 | 770.0 | 635.9 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.99 | 22.64 | -10.45 | 25.59 | 0.4033 | 937.0 | 768.3 | |
| 0.00 | 1.19 | 0.00 | 0.65 | 17.35 | 22.34 | -10.75 | 25.83 | 0.4104 | 818.0 | 606.9 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.78 | 22.25 | -10.85 | 26.67 | 0.4030 | 859.0 | 674.0 | |
| 0.00 | 1.87 | 0.00 | 1.01 | 17.06 | 22.17 | -10.92 | 26.51 | 0.4076 | 652.0 | 558.1 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 17.04 | 21.76 | -11.33 | 27.38 | 0.4102 | 732.0 | 552.5 | |
| 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. | |