| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.88 | 0.00 | 9.64 | 18.23 | 322.27 | 2.99 | 346.38 | 0.2404 | 605.0 | 436.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.74 | 0.00 | 0.88 | 13.16 | 326.00 | 6.72 | 320.43 | 0.1796 | 1023.0 | 842.9 | |
| 0.00 | 1.39 | 0.00 | 0.70 | 14.27 | 325.87 | 6.59 | 324.68 | 0.1934 | 889.0 | 614.6 | |
| 0.00 | 1.48 | 0.00 | 0.76 | 17.67 | 325.96 | 6.68 | 332.78 | 0.2433 | -869.0 | -584.5 | |
| 0.00 | 1.83 | 0.00 | 0.93 | 17.84 | 324.95 | 5.67 | 336.65 | 0.2385 | 885.0 | 775.9 | |
| 0.00 | 1.39 | 0.00 | 0.71 | 17.69 | 324.70 | 5.42 | 337.33 | 0.2345 | 887.0 | 675.8 | |
| 0.00 | 0.52 | 0.00 | 0.27 | 17.93 | 324.55 | 5.27 | 338.30 | 0.2374 | 934.0 | 790.8 | |
| 0.00 | 1.57 | 0.00 | 0.80 | 18.94 | 324.29 | 5.01 | 340.75 | 0.2519 | 979.0 | 750.3 | |
| 0.00 | 1.04 | 0.00 | 0.53 | 18.89 | 323.82 | 4.54 | 342.38 | 0.2484 | 692.0 | 542.6 | |
| 0.00 | 1.04 | 0.00 | 0.54 | 21.37 | 320.84 | 1.56 | 354.76 | 0.2798 | 884.0 | 730.4 | |
| 0.00 | 1.48 | 0.00 | 0.77 | 21.96 | 320.56 | 1.28 | 355.87 | 0.2893 | 765.0 | 508.8 | |
| 0.00 | 1.65 | 0.00 | 0.85 | 20.60 | 318.86 | -0.42 | 1.48 | 0.2656 | 866.0 | 611.1 | |
| 0.00 | 1.22 | 0.00 | 0.63 | 23.15 | 316.84 | -2.44 | 7.26 | 0.3109 | 750.0 | 587.1 | |
| 0.00 | 1.83 | 0.00 | 0.92 | 16.73 | 316.78 | -2.50 | 11.85 | 0.2040 | -928.0 | -743.2 | |
| 0.00 | 0.70 | 0.00 | 0.35 | 16.14 | 315.39 | -3.89 | 19.03 | 0.2007 | 713.0 | 533.8 | |
| 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. | |