| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.59 | 292.57 | 33.25 | 163.62 | -4.70 | 300.19 | -27.30 | 99.37 | 0.4653 | 480.8 | 341.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.99 | 5.97 | 0.55 | 3.31 | -5.94 | 301.32 | -26.17 | 102.49 | 0.4512 | 1120.4 | 703.2 | |
| 6.24 | 11.12 | 3.47 | 6.19 | -6.00 | 300.91 | -26.58 | 102.45 | 0.4577 | 1028.3 | 629.2 | |
| 37.08 | 203.39 | 20.61 | 113.07 | -4.20 | 300.75 | -26.74 | 98.48 | 0.4556 | 1300.2 | 432.7 | |
| 6.06 | 23.33 | 3.38 | 13.05 | -6.30 | 300.55 | -26.94 | 102.95 | 0.4640 | 1088.9 | 613.9 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -5.97 | 300.40 | -27.10 | 102.17 | 0.4653 | 906.0 | 583.1 | |
| 3.71 | -3.00 | 2.07 | -3.00 | -3.98 | 300.25 | -27.25 | 97.88 | 0.4629 | 752.2 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -5.48 | 300.15 | -27.35 | 101.04 | 0.4678 | 640.0 | 566.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -5.87 | 300.02 | -27.47 | 101.83 | 0.4707 | 580.0 | 497.6 | |
| 0.00 | 2.44 | 0.00 | 1.37 | -3.92 | 299.80 | -27.69 | 97.63 | 0.4697 | 714.0 | 540.5 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -3.19 | 299.83 | -27.67 | 96.08 | 0.4681 | 602.0 | 293.3 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -3.62 | 299.81 | -27.68 | 96.99 | 0.4690 | 220.0 | 277.1 | |
| 0.00 | 2.89 | 0.00 | 1.63 | -5.60 | 299.24 | -28.25 | 100.97 | 0.4818 | 699.0 | 597.1 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -5.26 | 299.26 | -28.23 | 100.29 | 0.4807 | 748.0 | 605.4 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -6.66 | 298.83 | -28.66 | 102.99 | 0.4909 | -867.0 | -680.9 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -6.54 | 298.70 | -28.80 | 102.69 | 0.4925 | -701.0 | -569.9 | |
| 1.99 | 3.53 | 1.13 | 2.01 | -6.45 | 298.46 | -29.04 | 102.42 | 0.4958 | -984.0 | -740.8 | |
| 0.00 | 1.27 | 0.00 | 0.72 | -6.17 | 298.23 | -29.26 | 101.79 | 0.4984 | -788.0 | -639.7 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -3.73 | 298.14 | -29.35 | 96.87 | 0.4946 | 855.0 | 742.8 | |
| 0.81 | 2.35 | 0.47 | 1.35 | -5.83 | 297.83 | -29.67 | 100.98 | 0.5035 | -854.1 | -631.6 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -3.88 | 297.75 | -29.74 | 97.09 | 0.5008 | 740.0 | 591.6 | |
| 0.81 | 2.35 | 0.47 | 1.35 | -3.79 | 297.61 | -29.88 | 96.88 | 0.5027 | 786.7 | 646.5 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -3.39 | 297.38 | -30.11 | 96.05 | 0.5056 | 622.0 | 532.5 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -8.13 | 296.95 | -30.54 | 105.06 | 0.5230 | -715.0 | -588.9 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -7.24 | 296.92 | -30.58 | 103.37 | 0.5207 | -738.0 | -683.9 | |
| 1.09 | 2.98 | 0.63 | 1.73 | -6.93 | 296.62 | -30.87 | 102.68 | 0.5242 | -892.2 | -670.7 | |
| 0.00 | 2.08 | 0.00 | 1.21 | -6.62 | 296.43 | -31.07 | 102.04 | 0.5262 | -571.0 | -459.1 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -6.13 | 296.35 | -31.14 | 101.10 | 0.5260 | -804.0 | -618.7 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -3.39 | 296.28 | -31.21 | 95.86 | 0.5221 | -748.0 | -583.8 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -7.79 | 296.01 | -31.48 | 104.05 | 0.5354 | -741.0 | -642.2 | |
| 0.00 | 2.44 | 0.00 | 1.42 | -5.12 | 296.16 | -31.33 | 99.14 | 0.5266 | -924.0 | -787.1 | |
| 0.00 | 1.27 | 0.00 | 0.74 | -4.36 | 296.13 | -31.36 | 97.69 | 0.5257 | -809.0 | -625.0 | |
| 0.00 | 2.35 | 0.00 | 1.38 | -6.71 | 295.88 | -31.61 | 102.03 | 0.5343 | -715.0 | -530.4 | |
| 0.81 | 1.63 | 0.47 | 0.95 | -4.94 | 295.96 | -31.53 | 98.74 | 0.5292 | -840.7 | -728.4 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -7.75 | 295.76 | -31.73 | 103.90 | 0.5389 | -445.0 | -364.3 | |
| 0.00 | 1.45 | 0.00 | 0.85 | -5.03 | 295.70 | -31.79 | 98.85 | 0.5332 | -579.0 | -429.9 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -8.31 | 295.39 | -32.11 | 104.76 | 0.5460 | -463.0 | -454.0 | |
| 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. | |