| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.15 | 287.64 | 25.68 | 159.02 | 16.87 | 354.33 | 22.85 | 303.01 | 0.4443 | -429.4 | -229.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.81 | 15.43 | 356.57 | 25.09 | 297.81 | 0.4640 | 639.0 | 491.8 | |
| 35.43 | 227.31 | 19.74 | 126.48 | 16.74 | 355.56 | 24.08 | 301.29 | 0.4590 | -1157.8 | -350.3 | |
| 10.72 | -2.00 | 5.94 | -2.00 | 16.88 | 354.74 | 23.26 | 302.37 | 0.4492 | -1178.6 | 999999 | |
| 0.00 | 2.91 | 0.00 | 1.59 | 14.49 | 353.91 | 22.43 | 298.26 | 0.4211 | -661.0 | -656.8 | |
| 0.00 | 3.09 | 0.00 | 1.70 | 17.05 | 354.04 | 22.55 | 303.44 | 0.4413 | -546.0 | -675.9 | |
| 0.00 | 1.82 | 0.00 | 1.02 | 19.67 | 354.37 | 22.89 | 308.02 | 0.4667 | -621.0 | -576.6 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 16.90 | 353.74 | 22.26 | 303.46 | 0.4362 | -919.0 | -812.4 | |
| 0.00 | 1.09 | 0.00 | 0.61 | 19.75 | 353.64 | 22.16 | 308.99 | 0.4586 | -819.0 | -618.2 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 15.92 | 352.57 | 21.08 | 302.74 | 0.4130 | -920.0 | -775.8 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 19.89 | 352.96 | 21.48 | 310.06 | 0.4518 | -691.0 | -505.2 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 16.05 | 352.38 | 20.89 | 303.24 | 0.4115 | -691.0 | -674.1 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 16.30 | 352.30 | 20.82 | 303.85 | 0.4125 | -833.0 | -722.8 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 20.03 | 352.29 | 20.81 | 311.15 | 0.4450 | -766.0 | -630.1 | |
| 0.00 | 1.64 | 0.00 | 0.90 | 20.19 | 352.14 | 20.66 | 311.64 | 0.4448 | -706.0 | -577.8 | |
| 0.00 | 1.73 | 0.00 | 0.95 | 19.41 | 351.62 | 20.13 | 310.88 | 0.4312 | -502.0 | -339.8 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 19.03 | 351.50 | 20.02 | 310.32 | 0.4262 | -843.0 | -713.0 | |
| 0.00 | 1.91 | 0.00 | 1.05 | 20.15 | 351.30 | 19.82 | 312.65 | 0.4346 | -801.0 | -687.2 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 12.77 | 350.00 | 18.52 | 298.43 | 0.3537 | 706.0 | 622.8 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 15.93 | 350.27 | 18.79 | 305.62 | 0.3827 | 732.0 | 650.8 | |
| 0.00 | 2.00 | 0.00 | 1.07 | 16.06 | 350.12 | 18.64 | 306.12 | 0.3817 | 838.0 | 712.7 | |
| 0.00 | 1.64 | 0.00 | 0.86 | 12.83 | 349.74 | 18.26 | 298.91 | 0.3505 | 940.0 | 737.9 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 16.10 | 349.95 | 18.47 | 306.42 | 0.3799 | 705.0 | 590.5 | |
| 0.00 | 1.64 | 0.00 | 0.89 | 19.69 | 350.24 | 18.76 | 313.29 | 0.4178 | -807.0 | -653.6 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 16.83 | 349.42 | 17.94 | 308.77 | 0.3798 | 857.0 | 774.5 | |
| 0.00 | 4.72 | 0.00 | 2.52 | 16.64 | 349.27 | 17.79 | 308.59 | 0.3761 | 1049.0 | 856.7 | |
| 0.00 | 2.54 | 0.00 | 1.36 | 16.99 | 349.24 | 17.76 | 309.39 | 0.3790 | 858.0 | 754.1 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 16.62 | 348.44 | 16.95 | 309.84 | 0.3654 | 920.0 | 697.0 | |
| 0.00 | 2.45 | 0.00 | 1.31 | 17.64 | 347.76 | 16.28 | 313.11 | 0.3675 | 838.0 | 758.1 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 17.30 | 347.57 | 16.08 | 312.72 | 0.3616 | 720.0 | 638.8 | |
| 0.00 | 3.82 | 0.00 | 2.02 | 17.24 | 347.39 | 15.91 | 312.88 | 0.3589 | 647.0 | 712.8 | |
| 0.00 | 1.73 | 0.00 | 0.92 | 18.38 | 346.93 | 15.45 | 316.06 | 0.3659 | 707.0 | 511.1 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 18.00 | 346.60 | 15.12 | 315.90 | 0.3579 | 851.0 | 694.2 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 18.16 | 346.51 | 15.03 | 316.38 | 0.3588 | 796.0 | 633.4 | |
| 0.00 | 2.00 | 0.00 | 1.05 | 17.25 | 346.14 | 14.66 | 315.18 | 0.3443 | 768.0 | 660.9 | |
| 0.00 | 2.09 | 0.00 | 1.10 | 16.69 | 345.99 | 14.51 | 314.22 | 0.3364 | 967.0 | 776.2 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 16.38 | 345.87 | 14.39 | 313.75 | 0.3315 | 815.0 | 662.1 | |
| 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. | |