| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 100.32 | 608.44 | 57.29 | 347.44 | -19.34 | 255.23 | 19.40 | 219.10 | 0.4991 | 721.0 | 350.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.91 | 0.00 | 0.58 | -21.24 | 266.19 | 30.37 | 228.88 | 0.6277 | 543.0 | 446.0 | |
| 0.00 | 0.36 | 0.00 | 0.23 | -19.95 | 265.35 | 29.52 | 229.82 | 0.6084 | 743.0 | 696.2 | |
| 0.00 | 1.64 | 0.00 | 1.05 | -23.17 | 265.31 | 29.49 | 225.66 | 0.6350 | 614.0 | 411.6 | |
| 0.00 | 2.36 | 0.00 | 1.47 | -20.92 | 264.62 | 28.79 | 227.86 | 0.6089 | 775.0 | 662.3 | |
| 0.00 | 0.91 | 0.00 | 0.57 | -21.53 | 264.59 | 28.77 | 227.06 | 0.6138 | 532.0 | 431.8 | |
| 1.18 | 5.81 | 0.72 | 3.54 | -20.95 | 262.15 | 26.32 | 225.39 | 0.5839 | 777.2 | 641.3 | |
| 0.00 | 0.55 | 0.00 | 0.32 | -21.83 | 256.19 | 20.36 | 217.25 | 0.5358 | -480.0 | -385.3 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -25.50 | 256.47 | 20.65 | 213.44 | 0.5797 | -716.0 | -579.7 | |
| 0.00 | 1.73 | 0.00 | 1.01 | -22.39 | 255.82 | 19.99 | 216.07 | 0.5390 | -77.0 | -135.4 | |
| 85.59 | 533.68 | 48.72 | 303.68 | -18.94 | 255.22 | 19.39 | 219.64 | 0.4942 | 1431.8 | 412.1 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -23.74 | 255.32 | 19.49 | 213.86 | 0.5503 | -777.0 | -610.7 | |
| 1.73 | 4.27 | 1.01 | 2.50 | -22.85 | 255.08 | 19.25 | 214.55 | 0.5379 | -945.8 | -775.3 | |
| 1.09 | -10.00 | 0.62 | -10.00 | -19.35 | 254.51 | 18.69 | 218.07 | 0.4922 | 1051.7 | 999999 | |
| 1.36 | 12.27 | 0.79 | 7.12 | -21.99 | 254.68 | 18.85 | 214.99 | 0.5245 | 448.1 | 58.4 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -22.60 | 254.73 | 18.90 | 214.35 | 0.5321 | -641.0 | -534.3 | |
| 0.82 | 2.54 | 0.47 | 1.47 | -21.45 | 254.43 | 18.61 | 215.29 | 0.5160 | 858.6 | 672.2 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -21.96 | 254.43 | 18.60 | 214.69 | 0.5220 | 642.0 | 525.8 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -20.94 | 254.19 | 18.37 | 215.57 | 0.5079 | 424.0 | 397.3 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -22.80 | 254.41 | 18.58 | 213.68 | 0.5318 | -886.0 | -729.1 | |
| 0.91 | 2.18 | 0.52 | 1.26 | -21.51 | 254.16 | 18.34 | 214.84 | 0.5144 | 782.5 | 647.6 | |
| 2.73 | 16.35 | 1.59 | 9.51 | -22.69 | 254.11 | 18.29 | 213.39 | 0.5281 | -942.4 | -658.0 | |
| 0.00 | 1.00 | 0.00 | 0.59 | -23.58 | 254.17 | 18.34 | 212.48 | 0.5392 | -690.0 | -498.2 | |
| 0.00 | 1.54 | 0.00 | 0.90 | -23.03 | 254.02 | 18.20 | 212.88 | 0.5314 | -650.0 | -481.0 | |
| 4.91 | -21.00 | 2.85 | -21.00 | -22.69 | 253.90 | 18.08 | 213.10 | 0.5263 | -1073.9 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.79 | -23.02 | 253.71 | 17.88 | 212.44 | 0.5288 | -604.0 | -421.3 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -20.84 | 252.67 | 16.85 | 213.43 | 0.4937 | 418.0 | 423.5 | |
| 0.00 | 2.18 | 0.00 | 1.23 | -20.50 | 252.23 | 16.40 | 213.14 | 0.4857 | 603.0 | 643.0 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -18.40 | 251.61 | 15.79 | 214.79 | 0.4542 | -635.0 | -531.5 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -18.99 | 251.53 | 15.71 | 213.89 | 0.4610 | -698.0 | -593.6 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -19.18 | 251.05 | 15.22 | 212.84 | 0.4592 | -671.0 | -550.1 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -20.24 | 250.75 | 14.92 | 211.05 | 0.4703 | -680.0 | -552.4 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -19.95 | 249.78 | 13.96 | 209.73 | 0.4591 | -669.0 | -556.8 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -19.81 | 249.07 | 13.24 | 208.63 | 0.4517 | -649.0 | -631.9 | |
| 0.00 | 1.09 | 0.00 | 0.61 | -21.51 | 248.95 | 13.13 | 206.59 | 0.4739 | -642.0 | -471.2 | |
| 0.00 | 1.09 | 0.00 | 0.65 | -27.93 | 249.34 | 13.51 | 201.63 | 0.5621 | -627.0 | -489.8 | |
| 0.00 | 1.09 | 0.00 | 0.64 | -26.57 | 246.48 | 10.66 | 198.28 | 0.5295 | -490.0 | -418.8 | |
| 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. | |