| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.42 | 0.00 | 10.95 | -15.22 | 76.24 | -31.48 | 112.67 | 0.5468 | -92.5 | -41.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.21 | 0.00 | 1.25 | -19.45 | 83.06 | -24.66 | 125.11 | 0.4829 | 566.0 | 511.5 | |
| 0.00 | 0.51 | 0.00 | 0.28 | -11.57 | 81.93 | -25.79 | 108.52 | 0.4513 | -616.0 | -596.7 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -10.92 | 81.19 | -26.53 | 106.75 | 0.4599 | -803.0 | -601.3 | |
| 0.00 | 1.19 | 0.00 | 0.67 | -13.57 | 79.98 | -27.74 | 111.50 | 0.4884 | -761.0 | -657.7 | |
| 0.00 | 1.19 | 0.00 | 0.68 | -13.30 | 78.88 | -28.84 | 110.35 | 0.5028 | -632.0 | -492.6 | |
| 0.00 | 0.76 | 0.00 | 0.45 | -16.11 | 77.54 | -30.18 | 114.78 | 0.5341 | 701.0 | 527.6 | |
| 0.00 | 1.44 | 0.00 | 0.85 | -16.59 | 77.17 | -30.55 | 115.39 | 0.5414 | 600.0 | 483.9 | |
| 0.00 | 1.70 | 0.00 | 0.99 | -13.19 | 77.50 | -30.22 | 109.45 | 0.5219 | -502.0 | -486.0 | |
| 0.00 | 1.70 | 0.00 | 1.00 | -15.23 | 76.40 | -31.32 | 112.58 | 0.5453 | 664.0 | 497.8 | |
| 0.00 | 1.53 | 0.00 | 0.93 | -18.53 | 74.34 | -33.38 | 116.99 | 0.5877 | 754.0 | 639.2 | |
| 0.00 | 1.10 | 0.00 | 0.69 | -20.82 | 72.75 | -34.97 | 119.64 | 0.6187 | 591.0 | 474.3 | |
| 0.00 | 2.29 | 0.00 | 1.38 | -11.00 | 73.69 | -34.03 | 104.05 | 0.5685 | -611.0 | -523.6 | |
| 0.00 | 0.85 | 0.00 | 0.55 | -11.53 | 67.60 | -40.12 | 103.44 | 0.6515 | -689.0 | -558.5 | |
| 0.00 | 0.42 | 0.00 | 0.38 | -23.43 | 52.58 | -55.13 | 115.72 | 0.8378 | -557.0 | -516.8 | |
| 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. | |