| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.59 | 62.80 | 11.17 | 38.27 | 5.62 | 69.51 | -35.54 | 86.12 | 0.5811 | 19.3 | 16.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.37 | 30.97 | 1.97 | 18.13 | 5.61 | 73.00 | -32.05 | 86.05 | 0.5315 | -1066.8 | -648.5 | |
| 6.75 | -1.00 | 3.95 | -1.00 | 5.79 | 72.82 | -32.24 | 85.73 | 0.5343 | -998.3 | 999999 | |
| 0.00 | 1.30 | 0.00 | 0.76 | 5.19 | 72.71 | -32.34 | 86.86 | 0.5357 | -743.0 | -547.7 | |
| 2.85 | -1.00 | 1.67 | -1.00 | 5.48 | 72.59 | -32.47 | 86.31 | 0.5376 | -779.6 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.72 | 4.56 | 71.25 | -33.81 | 88.00 | 0.5572 | -638.0 | -501.5 | |
| 0.00 | 1.04 | 0.00 | 0.62 | 5.13 | 71.18 | -33.87 | 86.98 | 0.5581 | -622.0 | -560.5 | |
| 0.00 | 1.90 | 0.00 | 1.20 | 6.06 | 67.00 | -38.05 | 85.47 | 0.6171 | 868.0 | 721.7 | |
| 0.00 | 1.64 | 0.00 | 1.03 | 6.26 | 66.83 | -38.22 | 85.15 | 0.6195 | 679.0 | 562.9 | |
| 0.00 | 0.87 | 0.00 | 0.55 | 6.15 | 66.38 | -38.67 | 85.34 | 0.6256 | 682.0 | 638.4 | |
| 0.00 | 3.63 | 0.00 | 2.31 | 6.05 | 66.12 | -38.93 | 85.51 | 0.6291 | 713.0 | 571.0 | |
| 4.15 | 7.35 | 2.64 | 4.68 | 5.63 | 66.08 | -38.97 | 86.18 | 0.6296 | 846.1 | 585.7 | |
| 0.00 | 1.56 | 0.00 | 0.99 | 7.00 | 65.96 | -39.09 | 84.01 | 0.6316 | 755.0 | 624.1 | |
| 0.00 | 1.73 | 0.00 | 1.10 | 5.30 | 66.07 | -38.99 | 86.70 | 0.6298 | 732.0 | 489.1 | |
| 0.69 | 2.94 | 0.44 | 1.88 | 5.08 | 65.85 | -39.20 | 87.05 | 0.6327 | 766.9 | 651.3 | |
| 0.00 | 0.78 | 0.00 | 0.50 | 5.43 | 65.59 | -39.46 | 86.50 | 0.6362 | 579.0 | 473.6 | |
| 0.00 | 1.99 | 0.00 | 1.27 | 4.24 | 65.60 | -39.46 | 88.38 | 0.6363 | 592.0 | 411.5 | |
| 0.78 | 3.20 | 0.50 | 2.08 | 5.51 | 64.73 | -40.33 | 86.37 | 0.6477 | 786.0 | 660.2 | |
| 0.00 | 0.69 | 0.00 | 0.45 | 5.35 | 64.54 | -40.51 | 86.62 | 0.6502 | 484.0 | 431.9 | |
| 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. | |