| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.71 | 0.00 | 12.66 | 18.66 | 357.23 | -7.62 | 27.79 | 0.2479 | -403.1 | -325.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.15 | 0.00 | 1.08 | 14.50 | 4.55 | -0.30 | 2.23 | 0.1301 | -835.0 | -768.9 | |
| 0.00 | 2.42 | 0.00 | 1.22 | 17.77 | 1.81 | -3.04 | 15.19 | 0.1936 | -1110.0 | -859.2 | |
| 0.00 | 0.54 | 0.00 | 0.27 | 20.06 | 1.05 | -3.79 | 15.43 | 0.2346 | -863.0 | -675.2 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 20.15 | 0.60 | -4.25 | 17.05 | 0.2382 | -845.0 | -668.5 | |
| 0.00 | 3.95 | 0.00 | 2.01 | 19.80 | 0.19 | -4.66 | 19.08 | 0.2348 | -1081.0 | -890.0 | |
| 0.00 | 1.71 | 0.00 | 0.86 | 16.93 | 0.23 | -4.61 | 24.14 | 0.1890 | -888.0 | -748.7 | |
| 0.00 | 1.62 | 0.00 | 0.82 | 19.55 | 359.94 | -4.91 | 20.42 | 0.2322 | -1017.0 | -800.0 | |
| 0.00 | 1.08 | 0.00 | 0.54 | 17.57 | 359.87 | -4.98 | 24.36 | 0.2016 | -814.0 | -741.2 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 19.89 | 359.80 | -5.05 | 20.41 | 0.2384 | -702.0 | -502.7 | |
| 0.00 | 0.99 | 0.00 | 0.50 | 15.46 | 357.87 | -6.98 | 38.57 | 0.1887 | -809.0 | -605.3 | |
| 0.00 | 1.62 | 0.00 | 0.83 | 17.76 | 354.14 | -10.70 | 43.32 | 0.2589 | 906.0 | 755.4 | |
| 0.00 | 1.26 | 0.00 | 0.64 | 15.09 | 353.24 | -11.61 | 53.82 | 0.2418 | 737.0 | 610.6 | |
| 0.00 | 3.32 | 0.00 | 1.79 | 22.93 | 347.39 | -17.46 | 44.77 | 0.3940 | 854.0 | 603.2 | |
| 0.00 | 1.35 | 0.00 | 0.72 | 17.80 | 345.60 | -19.25 | 58.43 | 0.3700 | 823.0 | 623.3 | |
| 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. | |