| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.33 | 538.13 | 52.45 | 308.82 | 4.01 | 245.44 | -28.58 | 71.65 | 0.5039 | -336.2 | -232.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.77 | 416.63 | 37.69 | 235.25 | 3.98 | 247.03 | -27.00 | 70.80 | 0.4815 | -1301.2 | -429.3 | |
| 0.00 | 2.74 | 0.00 | 1.54 | 1.69 | 246.54 | -27.49 | 75.67 | 0.4781 | -857.0 | -725.8 | |
| 2.12 | -1.00 | 1.20 | -1.00 | 3.71 | 246.32 | -27.71 | 71.81 | 0.4903 | -598.3 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.65 | 1.80 | 245.58 | -28.44 | 75.98 | 0.4927 | -541.0 | -418.1 | |
| 6.80 | 17.75 | 3.90 | 10.19 | 3.97 | 245.35 | -28.67 | 71.93 | 0.5055 | -889.2 | -480.5 | |
| 0.00 | 1.94 | 0.00 | 1.13 | 4.40 | 244.02 | -30.01 | 71.95 | 0.5265 | -749.0 | -558.6 | |
| 0.00 | 0.88 | 0.00 | 0.52 | 4.60 | 243.77 | -30.26 | 71.75 | 0.5310 | -611.0 | -497.3 | |
| 0.00 | 1.85 | 0.00 | 1.09 | 2.23 | 242.41 | -31.62 | 76.72 | 0.5404 | 763.0 | 589.3 | |
| 0.00 | 0.79 | 0.00 | 0.47 | 2.83 | 242.14 | -31.88 | 75.78 | 0.5463 | -296.0 | -169.4 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 2.78 | 241.93 | -32.09 | 75.97 | 0.5491 | 697.0 | 472.0 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 4.70 | 241.82 | -32.21 | 72.68 | 0.5586 | 910.0 | 663.9 | |
| 0.00 | 4.59 | 0.00 | 2.73 | 3.73 | 241.83 | -32.20 | 74.36 | 0.5543 | 842.0 | 801.9 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 3.74 | 241.58 | -32.45 | 74.46 | 0.5579 | 766.0 | 592.0 | |
| 0.00 | 1.59 | 0.00 | 0.95 | 3.47 | 241.55 | -32.47 | 74.94 | 0.5571 | 891.0 | 713.7 | |
| 0.00 | 1.85 | 0.00 | 1.11 | 3.76 | 241.15 | -32.88 | 74.63 | 0.5640 | 873.0 | 731.2 | |
| 0.00 | 2.38 | 0.00 | 1.43 | 3.49 | 241.05 | -32.98 | 75.14 | 0.5643 | 940.0 | 728.5 | |
| 0.71 | 3.36 | 0.42 | 2.02 | 4.20 | 240.95 | -33.08 | 73.98 | 0.5685 | 915.9 | 771.7 | |
| 0.00 | 1.06 | 0.00 | 0.64 | 3.71 | 240.93 | -33.09 | 74.82 | 0.5668 | 756.0 | 642.8 | |
| 0.00 | 1.41 | 0.00 | 0.85 | 2.51 | 240.79 | -33.23 | 76.95 | 0.5642 | 692.0 | 497.1 | |
| 0.00 | 1.50 | 0.00 | 0.90 | 3.24 | 240.66 | -33.36 | 75.75 | 0.5687 | 922.0 | 792.8 | |
| 0.00 | 1.50 | 0.00 | 0.91 | 3.26 | 240.41 | -33.62 | 75.84 | 0.5723 | 781.0 | 688.1 | |
| 0.00 | 1.68 | 0.00 | 1.02 | 3.88 | 240.09 | -33.93 | 74.93 | 0.5790 | 697.0 | 588.6 | |
| 0.71 | 3.89 | 0.43 | 2.36 | 4.29 | 239.93 | -34.10 | 74.33 | 0.5828 | 855.2 | 632.2 | |
| 0.00 | 2.56 | 0.00 | 1.56 | 4.90 | 239.90 | -34.13 | 73.34 | 0.5858 | 674.0 | 654.8 | |
| 1.68 | 5.65 | 1.02 | 3.44 | 4.54 | 239.84 | -34.19 | 73.96 | 0.5850 | 821.2 | 617.0 | |
| 0.00 | 3.80 | 0.00 | 2.33 | 5.17 | 239.44 | -34.59 | 73.12 | 0.5930 | 741.0 | 640.7 | |
| 0.00 | 1.41 | 0.00 | 0.87 | 5.63 | 238.97 | -35.06 | 72.62 | 0.6012 | 846.0 | 731.3 | |
| 0.00 | 3.00 | 0.00 | 1.86 | 6.00 | 238.87 | -35.16 | 72.08 | 0.6041 | 712.0 | 608.5 | |
| 0.00 | 0.97 | 0.00 | 0.60 | 6.26 | 238.74 | -35.29 | 71.75 | 0.6070 | 574.0 | 398.3 | |
| 0.00 | 1.59 | 0.00 | 0.99 | 5.56 | 238.60 | -35.43 | 72.92 | 0.6058 | 834.0 | 724.6 | |
| 0.00 | 2.38 | 0.00 | 1.49 | 6.00 | 238.35 | -35.68 | 72.34 | 0.6110 | 564.0 | 619.5 | |
| 5.30 | 43.10 | 3.29 | 26.81 | 4.23 | 238.35 | -35.68 | 75.15 | 0.6040 | 1016.1 | 534.8 | |
| 0.79 | -32.00 | 0.49 | -32.00 | 4.02 | 238.32 | -35.71 | 75.50 | 0.6036 | 1041.4 | 999999 | |
| 4.15 | -32.00 | 2.58 | -32.00 | 4.13 | 238.05 | -35.97 | 75.44 | 0.6076 | 993.0 | 999999 | |
| 2.30 | -32.00 | 1.43 | -32.00 | 4.29 | 237.86 | -36.17 | 75.27 | 0.6108 | 703.3 | 999999 | |
| 0.00 | 0.71 | 0.00 | 0.44 | 2.76 | 237.51 | -36.51 | 77.85 | 0.6102 | 619.0 | 544.0 | |
| 0.00 | 1.24 | 0.00 | 0.78 | 4.14 | 236.85 | -37.18 | 75.92 | 0.6236 | 646.0 | 554.1 | |
| 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. | |