| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.32 | 29.41 | 0.77 | 16.83 | -8.66 | 9.49 | 30.01 | 262.69 | 0.5011 | 329.9 | 296.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.72 | -8.26 | 12.18 | 32.70 | 264.18 | 0.5396 | 464.0 | 423.6 | |
| 0.00 | 0.44 | 0.00 | 0.26 | -7.88 | 11.90 | 32.42 | 264.87 | 0.5353 | 535.0 | 478.2 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -9.06 | 11.90 | 32.42 | 262.67 | 0.5359 | 537.0 | 374.0 | |
| 0.00 | 4.05 | 0.00 | 2.37 | -8.85 | 11.84 | 32.36 | 263.05 | 0.5349 | 620.0 | 548.8 | |
| 0.00 | 2.73 | 0.00 | 1.59 | -5.19 | 11.53 | 32.05 | 269.94 | 0.5305 | 705.0 | 582.2 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -8.52 | 11.70 | 32.22 | 263.65 | 0.5327 | 753.0 | 579.5 | |
| 1.32 | 4.23 | 0.77 | 2.47 | -8.20 | 11.60 | 32.12 | 264.26 | 0.5310 | 912.0 | 688.3 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -8.54 | 11.45 | 31.97 | 263.60 | 0.5290 | 780.0 | 603.6 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -11.83 | 10.84 | 31.37 | 257.25 | 0.5244 | -652.0 | -549.6 | |
| 0.00 | 2.91 | 0.00 | 1.67 | -7.89 | 9.98 | 30.50 | 264.76 | 0.5068 | 832.0 | 709.7 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -10.18 | 9.45 | 29.97 | 260.15 | 0.5010 | 509.0 | 343.8 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -10.36 | 9.43 | 29.95 | 259.78 | 0.5010 | 494.0 | 443.5 | |
| 0.00 | 1.32 | 0.00 | 0.73 | -7.61 | 6.63 | 27.15 | 265.18 | 0.4558 | -780.0 | -655.8 | |
| 0.00 | 3.61 | 0.00 | 2.00 | -7.53 | 6.32 | 26.84 | 265.33 | 0.4510 | -641.0 | -488.3 | |
| 0.00 | 2.47 | 0.00 | 1.30 | -14.52 | 358.36 | 18.88 | 244.09 | 0.3498 | 14.0 | -3.6 | |
| 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. | |