| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.77 | 452.21 | 45.96 | 283.05 | 17.07 | 169.18 | 35.00 | 296.14 | 0.6122 | -571.3 | -271.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.71 | 14.19 | 173.29 | 39.11 | 289.80 | 0.6522 | -596.0 | -512.9 | |
| 0.00 | 1.09 | 0.00 | 0.69 | 12.91 | 171.37 | 37.19 | 288.56 | 0.6237 | -640.0 | -443.0 | |
| 0.00 | 1.18 | 0.00 | 0.76 | 16.88 | 172.10 | 37.92 | 294.29 | 0.6475 | -649.0 | -479.8 | |
| 71.68 | 394.13 | 45.28 | 248.90 | 17.05 | 170.03 | 35.85 | 295.54 | 0.6227 | -1318.0 | -381.0 | |
| 1.09 | -4.00 | 0.68 | -4.00 | 16.40 | 169.42 | 35.23 | 294.85 | 0.6122 | -1242.8 | 999999 | |
| 0.00 | 2.54 | 0.00 | 1.56 | 16.36 | 168.09 | 33.91 | 295.49 | 0.5953 | -782.0 | -681.3 | |
| 0.00 | 1.09 | 0.00 | 0.67 | 16.55 | 167.83 | 33.64 | 295.95 | 0.5928 | -715.0 | -495.9 | |
| 0.00 | 3.18 | 0.00 | 1.97 | 17.97 | 168.08 | 33.90 | 298.03 | 0.6033 | -645.0 | -503.1 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 18.30 | 167.46 | 33.28 | 298.91 | 0.5974 | -167.0 | -224.8 | |
| 0.00 | 1.00 | 0.00 | 0.61 | 18.63 | 166.99 | 32.81 | 299.71 | 0.5934 | 343.0 | 352.1 | |
| 0.00 | 1.27 | 0.00 | 0.77 | 16.64 | 166.55 | 32.37 | 296.84 | 0.5770 | 449.0 | 397.9 | |
| 0.00 | 4.54 | 0.00 | 2.70 | 16.85 | 164.76 | 30.58 | 298.35 | 0.5553 | 567.0 | 539.2 | |
| 0.00 | 1.81 | 0.00 | 1.08 | 16.57 | 164.67 | 30.49 | 297.94 | 0.5526 | 805.0 | 602.2 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 18.04 | 164.02 | 29.83 | 300.83 | 0.5530 | 661.0 | 462.7 | |
| 0.00 | 1.18 | 0.00 | 0.70 | 16.93 | 163.82 | 29.63 | 299.14 | 0.5437 | 817.0 | 616.0 | |
| 0.00 | 2.27 | 0.00 | 1.36 | 19.09 | 164.14 | 29.96 | 302.43 | 0.5614 | 564.0 | 476.5 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 17.76 | 163.59 | 29.41 | 300.69 | 0.5460 | 818.0 | 710.1 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 15.59 | 162.98 | 28.80 | 297.44 | 0.5248 | 799.0 | 624.1 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 18.08 | 163.29 | 29.11 | 301.46 | 0.5442 | 571.0 | 524.8 | |
| 0.00 | 2.09 | 0.00 | 1.22 | 17.87 | 162.88 | 28.70 | 301.42 | 0.5377 | 778.0 | 673.7 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 17.61 | 162.84 | 28.66 | 301.03 | 0.5354 | 851.0 | 690.6 | |
| 0.00 | 1.91 | 0.00 | 1.11 | 17.77 | 162.65 | 28.46 | 301.45 | 0.5341 | 702.0 | 705.5 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 18.82 | 162.80 | 28.62 | 303.06 | 0.5430 | 694.0 | 556.9 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 18.03 | 162.65 | 28.47 | 301.87 | 0.5359 | 594.0 | 479.7 | |
| 0.00 | 1.09 | 0.00 | 0.67 | 24.46 | 163.67 | 29.49 | 310.87 | 0.5948 | 673.0 | 569.0 | |
| 0.00 | 1.36 | 0.00 | 0.78 | 16.91 | 161.13 | 26.95 | 301.20 | 0.5090 | 821.0 | 638.0 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 19.67 | 161.28 | 27.09 | 305.77 | 0.5306 | 608.0 | 475.9 | |
| 0.00 | 1.27 | 0.00 | 0.72 | 16.64 | 160.10 | 25.91 | 301.63 | 0.4937 | 684.0 | 467.6 | |
| 0.00 | 1.81 | 0.00 | 1.04 | 17.59 | 160.17 | 25.99 | 303.25 | 0.5014 | 1000.0 | 747.6 | |
| 0.00 | 1.72 | 0.00 | 0.99 | 17.75 | 160.12 | 25.94 | 303.57 | 0.5020 | 800.0 | 548.6 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 17.69 | 159.93 | 25.75 | 303.64 | 0.4992 | 816.0 | 685.6 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 20.98 | 160.28 | 26.10 | 308.79 | 0.5291 | 559.0 | 534.5 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 19.15 | 159.88 | 25.70 | 306.20 | 0.5097 | 689.0 | 611.5 | |
| 0.00 | 1.72 | 0.00 | 0.97 | 15.52 | 159.13 | 24.95 | 300.42 | 0.4733 | 688.0 | 686.7 | |
| 0.00 | 6.08 | 0.00 | 3.35 | 15.36 | 156.76 | 22.58 | 302.46 | 0.4406 | 826.0 | 728.3 | |
| 0.00 | 3.99 | 0.00 | 2.22 | 17.09 | 156.77 | 22.59 | 305.80 | 0.4545 | 861.0 | 581.0 | |
| 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. | |