| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 34.32 | 0.00 | 18.41 | 6.84 | 264.67 | -20.23 | 78.29 | 0.3505 | 209.4 | 291.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.59 | 2.37 | 280.05 | -4.85 | 98.76 | 0.0859 | -816.0 | -651.9 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 7.40 | 279.34 | -5.56 | 52.15 | 0.1223 | -801.0 | -647.7 | |
| 0.00 | 3.09 | 0.00 | 1.54 | 3.59 | 278.79 | -6.12 | 85.56 | 0.1071 | -942.0 | -754.1 | |
| 0.00 | 1.36 | 0.00 | 0.68 | 4.27 | 276.16 | -8.74 | 82.28 | 0.1536 | -872.0 | -728.1 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 4.03 | 275.92 | -8.98 | 84.03 | 0.1573 | -821.0 | -581.8 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 1.57 | 273.92 | -10.98 | 97.84 | 0.1930 | -764.0 | -596.5 | |
| 0.00 | 4.09 | 0.00 | 2.11 | 9.21 | 269.35 | -15.55 | 67.82 | 0.2871 | 863.0 | 748.9 | |
| 0.00 | 2.09 | 0.00 | 1.10 | 11.47 | 266.27 | -18.63 | 64.72 | 0.3477 | 600.0 | 388.3 | |
| 0.00 | 1.73 | 0.00 | 0.91 | 9.61 | 265.21 | -19.69 | 70.76 | 0.3534 | 753.0 | 596.2 | |
| 0.00 | 1.63 | 0.00 | 0.89 | 8.83 | 261.34 | -23.57 | 75.28 | 0.4102 | 859.0 | 653.2 | |
| 0.00 | 3.72 | 0.00 | 2.02 | 8.67 | 261.08 | -23.82 | 75.78 | 0.4137 | 855.0 | 736.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 8.94 | 260.52 | -24.38 | 75.44 | 0.4231 | 744.0 | 610.7 | |
| 0.00 | 2.36 | 0.00 | 1.31 | 7.39 | 258.37 | -26.53 | 79.77 | 0.4520 | 752.0 | 562.6 | |
| 0.00 | 2.27 | 0.00 | 1.26 | 7.72 | 257.97 | -26.93 | 79.18 | 0.4588 | 806.0 | 656.1 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 8.02 | 257.91 | -26.99 | 78.54 | 0.4604 | 659.0 | 521.2 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 5.09 | 255.65 | -29.25 | 85.16 | 0.4904 | 732.0 | 647.7 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 0.63 | 254.18 | -30.72 | 94.02 | 0.5141 | 623.0 | 508.8 | |
| 0.00 | 2.81 | 0.00 | 1.72 | 4.55 | 249.21 | -35.69 | 86.56 | 0.5848 | 539.0 | 500.0 | |
| 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. | |