| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.72 | 49.58 | 8.94 | 25.15 | 14.97 | 24.71 | -0.26 | 0.47 | 0.2125 | -145.1 | -424.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.08 | 15.62 | 6.59 | 7.87 | 13.26 | 26.42 | 1.45 | 352.26 | 0.1834 | 1042.2 | 795.2 | |
| 0.00 | 3.63 | 0.00 | 1.84 | 15.38 | 25.17 | 0.20 | 359.12 | 0.2181 | -836.0 | -673.9 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 16.04 | 24.98 | 0.01 | 359.96 | 0.2293 | -879.0 | -717.6 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 16.19 | 24.98 | 0.01 | 359.97 | 0.2320 | -767.0 | -624.6 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 16.19 | 24.85 | -0.12 | 0.49 | 0.2320 | -931.0 | -763.2 | |
| 1.64 | 2.36 | 0.83 | 1.20 | 16.38 | 24.66 | -0.31 | 1.27 | 0.2352 | -1018.0 | -1033.5 | |
| 1.91 | 2.36 | 0.96 | 1.19 | 14.38 | 24.48 | -0.49 | 2.39 | 0.2012 | -981.3 | -800.4 | |
| 0.00 | 3.54 | 0.00 | 1.80 | 15.88 | 24.41 | -0.56 | 2.39 | 0.2268 | -903.0 | -709.2 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 16.66 | 24.41 | -0.56 | 2.26 | 0.2402 | -848.0 | -788.2 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 14.07 | 24.35 | -0.62 | 3.08 | 0.1959 | -793.0 | -570.7 | |
| 0.00 | 1.82 | 0.00 | 0.92 | 13.42 | 24.23 | -0.74 | 3.93 | 0.1848 | 948.0 | 648.3 | |
| 0.00 | 5.90 | 0.00 | 3.00 | 15.22 | 23.97 | -1.00 | 4.50 | 0.2161 | -1227.0 | -904.5 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 15.28 | 23.78 | -1.19 | 5.32 | 0.2174 | -873.0 | -696.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 14.85 | 23.63 | -1.35 | 6.23 | 0.2102 | -806.0 | -620.8 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 17.13 | 23.29 | -1.68 | 6.48 | 0.2496 | -999.0 | -844.1 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 17.35 | 22.68 | -2.29 | 8.66 | 0.2546 | -732.0 | -496.9 | |
| 1.09 | 2.00 | 0.56 | 1.03 | 17.98 | 21.55 | -3.42 | 12.26 | 0.2685 | 638.1 | 623.7 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 17.63 | 20.76 | -4.22 | 15.34 | 0.2660 | 879.0 | 682.3 | |
| 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. | |