| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.80 | 447.58 | 39.88 | 286.35 | 17.01 | 169.30 | 36.79 | 295.12 | 0.6338 | -445.0 | -290.5 | |
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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 | 0.72 | 11.56 | 173.42 | 40.90 | 285.31 | 0.6674 | -545.0 | -471.5 | |
| 0.00 | 1.36 | 0.00 | 0.90 | 16.74 | 172.18 | 39.66 | 293.32 | 0.6678 | -560.0 | -434.9 | |
| 0.00 | 1.09 | 0.00 | 0.73 | 17.88 | 172.43 | 39.91 | 294.83 | 0.6751 | 569.0 | 495.5 | |
| 0.00 | 2.18 | 0.00 | 1.43 | 16.06 | 171.80 | 39.28 | 292.47 | 0.6607 | 449.0 | 429.8 | |
| 61.80 | 400.21 | 39.88 | 258.15 | 17.01 | 170.03 | 37.52 | 294.64 | 0.6429 | -1247.9 | -384.9 | |
| 0.00 | 0.36 | 0.00 | 0.23 | 13.92 | 168.64 | 36.12 | 290.54 | 0.6133 | -387.0 | -443.0 | |
| 0.00 | 0.27 | 0.00 | 0.17 | 15.97 | 168.02 | 35.50 | 294.03 | 0.6136 | -339.0 | -439.0 | |
| 0.00 | 1.00 | 0.00 | 0.63 | 16.26 | 168.00 | 35.49 | 294.48 | 0.6146 | -876.0 | -772.8 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 16.42 | 167.88 | 35.36 | 294.79 | 0.6137 | -646.0 | -570.7 | |
| 0.00 | 0.73 | 0.00 | 0.45 | 16.73 | 166.44 | 33.92 | 296.05 | 0.5970 | 495.0 | 400.8 | |
| 0.00 | 0.54 | 0.00 | 0.33 | 17.01 | 164.85 | 32.33 | 297.43 | 0.5784 | 636.0 | 581.7 | |
| 0.00 | 2.09 | 0.00 | 1.26 | 16.53 | 164.73 | 32.21 | 296.74 | 0.5743 | 719.0 | 539.2 | |
| 0.00 | 1.27 | 0.00 | 0.77 | 16.76 | 164.54 | 32.02 | 297.22 | 0.5731 | 480.0 | 396.6 | |
| 0.00 | 1.18 | 0.00 | 0.71 | 17.46 | 164.30 | 31.78 | 298.51 | 0.5739 | 634.0 | 460.3 | |
| 0.00 | 1.09 | 0.00 | 0.66 | 18.07 | 164.08 | 31.56 | 299.63 | 0.5746 | 590.0 | 491.3 | |
| 0.00 | 2.09 | 0.00 | 1.25 | 17.76 | 163.61 | 31.09 | 299.45 | 0.5669 | 720.0 | 557.5 | |
| 0.00 | 2.90 | 0.00 | 1.74 | 18.17 | 163.28 | 30.76 | 300.36 | 0.5653 | 601.0 | 511.0 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 18.46 | 163.19 | 30.67 | 300.89 | 0.5659 | 612.0 | 529.4 | |
| 0.00 | 1.54 | 0.00 | 0.92 | 17.67 | 162.96 | 30.44 | 299.77 | 0.5582 | 870.0 | 703.0 | |
| 0.00 | 1.72 | 0.00 | 1.03 | 17.80 | 162.76 | 30.24 | 300.12 | 0.5565 | 736.0 | 605.2 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 18.75 | 162.87 | 30.35 | 301.58 | 0.5638 | 681.0 | 511.9 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 17.07 | 161.20 | 28.68 | 300.05 | 0.5321 | 955.0 | 813.7 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 17.56 | 160.19 | 27.67 | 301.69 | 0.5224 | 793.0 | 709.3 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 17.71 | 160.18 | 27.66 | 301.97 | 0.5234 | 681.0 | 603.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 15.67 | 159.50 | 26.99 | 298.93 | 0.5012 | 793.0 | 586.9 | |
| 0.00 | 0.73 | 0.00 | 0.41 | 15.46 | 159.30 | 26.78 | 298.70 | 0.4970 | 729.0 | 672.8 | |
| 0.00 | 1.36 | 0.00 | 0.79 | 19.15 | 159.85 | 27.33 | 304.67 | 0.5294 | 706.0 | 560.5 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 18.20 | 159.22 | 26.70 | 303.64 | 0.5147 | 837.0 | 745.2 | |
| 0.00 | 1.00 | 0.00 | 0.58 | 19.46 | 158.75 | 26.23 | 306.18 | 0.5183 | 567.0 | 459.0 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 19.75 | 158.26 | 25.74 | 307.14 | 0.5147 | 635.0 | 491.4 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 23.77 | 158.45 | 25.94 | 313.17 | 0.5510 | 569.0 | 427.4 | |
| 0.00 | 1.36 | 0.00 | 0.77 | 17.34 | 157.24 | 24.72 | 303.99 | 0.4833 | 692.0 | 584.5 | |
| 0.00 | 3.99 | 0.00 | 2.23 | 15.43 | 156.84 | 24.32 | 300.80 | 0.4640 | 937.0 | 772.8 | |
| 0.00 | 2.18 | 0.00 | 1.23 | 17.25 | 156.91 | 24.39 | 304.15 | 0.4784 | 690.0 | 623.8 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 14.48 | 155.21 | 22.69 | 300.51 | 0.4354 | 723.0 | 554.9 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 15.00 | 153.60 | 21.08 | 303.35 | 0.4177 | 696.0 | 626.0 | |
| 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. | |