| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.72 | 272.55 | 21.22 | 138.63 | -4.26 | 302.43 | 12.45 | 251.12 | 0.2285 | 861.2 | 437.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.90 | 0.00 | 0.98 | -4.96 | 304.32 | 14.34 | 250.93 | 0.2622 | 988.0 | 814.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | -5.36 | 304.14 | 14.16 | 249.27 | 0.2616 | 786.0 | 647.1 | |
| 0.00 | 5.16 | 0.00 | 2.64 | -6.46 | 303.54 | 13.56 | 244.46 | 0.2593 | 454.0 | 512.0 | |
| 0.00 | 1.63 | 0.00 | 0.83 | -5.39 | 303.45 | 13.47 | 248.21 | 0.2508 | 989.0 | 808.9 | |
| 34.93 | 224.68 | 17.77 | 114.32 | -4.01 | 302.61 | 12.63 | 252.49 | 0.2297 | 1367.3 | 443.2 | |
| 6.79 | 17.28 | 3.45 | 8.80 | -5.48 | 302.07 | 12.09 | 245.67 | 0.2299 | 1117.4 | 694.2 | |
| 0.00 | 1.81 | 0.00 | 0.92 | -5.78 | 301.67 | 11.69 | 243.72 | 0.2259 | 1001.0 | 854.4 | |
| 0.00 | 2.26 | 0.00 | 1.15 | -5.81 | 301.46 | 11.47 | 243.17 | 0.2228 | 802.0 | 641.8 | |
| 0.00 | 2.53 | 0.00 | 1.28 | -4.41 | 301.40 | 11.42 | 249.02 | 0.2123 | 976.0 | 707.4 | |
| 0.00 | 2.71 | 0.00 | 1.38 | -4.62 | 301.37 | 11.39 | 248.03 | 0.2132 | 704.0 | 537.4 | |
| 0.00 | 1.00 | 0.00 | 0.50 | -3.19 | 300.83 | 10.84 | 253.84 | 0.1965 | 589.0 | 450.9 | |
| 0.00 | 1.18 | 0.00 | 0.59 | -5.35 | 300.27 | 10.28 | 242.60 | 0.2011 | -748.0 | -514.5 | |
| 0.00 | 1.99 | 0.00 | 1.00 | -3.89 | 299.72 | 9.74 | 248.45 | 0.1822 | 785.0 | 673.1 | |
| 0.00 | 0.36 | 0.00 | 0.18 | -2.91 | 299.56 | 9.57 | 253.36 | 0.1741 | -377.0 | -436.5 | |
| 0.00 | 1.90 | 0.00 | 0.96 | -6.73 | 299.20 | 9.22 | 233.91 | 0.1978 | -747.0 | -460.6 | |
| 0.00 | 1.63 | 0.00 | 0.82 | -5.23 | 298.68 | 8.70 | 239.16 | 0.1763 | -635.0 | -578.2 | |
| 0.00 | 2.26 | 0.00 | 1.14 | -7.55 | 297.67 | 7.68 | 225.50 | 0.1867 | -827.0 | -681.1 | |
| 0.00 | 1.09 | 0.00 | 0.54 | -3.43 | 297.53 | 7.54 | 245.90 | 0.1442 | -840.0 | -674.3 | |
| 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. | |