| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.50 | 0.00 | 14.65 | -17.95 | 328.10 | 6.77 | 209.96 | 0.2671 | 266.6 | 310.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.94 | 0.00 | 1.01 | -15.31 | 336.63 | 15.30 | 236.93 | 0.3051 | 776.0 | 665.0 | |
| 0.00 | 2.82 | 0.00 | 1.44 | -15.49 | 332.39 | 11.06 | 227.86 | 0.2504 | 948.0 | 778.3 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -16.19 | 332.43 | 11.09 | 225.87 | 0.2586 | 786.0 | 581.3 | |
| 0.00 | 1.24 | 0.00 | 0.63 | -14.37 | 332.27 | 10.94 | 231.19 | 0.2369 | 922.0 | 762.0 | |
| 0.00 | 4.85 | 0.00 | 2.48 | -14.64 | 332.25 | 10.92 | 230.22 | 0.2395 | 1042.0 | 819.3 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -14.44 | 331.83 | 10.50 | 229.84 | 0.2319 | 759.0 | 687.8 | |
| 0.00 | 4.06 | 0.00 | 2.08 | -17.00 | 331.77 | 10.44 | 221.93 | 0.2605 | 679.0 | 457.1 | |
| 0.00 | 1.68 | 0.00 | 0.86 | -17.80 | 329.35 | 8.02 | 212.83 | 0.2462 | 967.0 | 758.3 | |
| 0.00 | 1.85 | 0.00 | 0.95 | -17.59 | 329.19 | 7.85 | 212.78 | 0.2417 | 802.0 | 537.3 | |
| 0.00 | 3.18 | 0.00 | 1.64 | -22.56 | 320.43 | -0.90 | 177.09 | 0.2871 | -849.0 | -551.0 | |
| 0.00 | 1.50 | 0.00 | 0.77 | -22.40 | 319.88 | -1.45 | 175.27 | 0.2851 | -825.0 | -584.3 | |
| 0.00 | 1.68 | 0.00 | 0.88 | -23.89 | 316.80 | -4.53 | 166.81 | 0.3177 | -676.0 | -599.3 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -24.07 | 315.87 | -5.46 | 164.40 | 0.3244 | -725.0 | -617.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | -23.71 | 312.95 | -8.38 | 156.41 | 0.3351 | -873.0 | -702.7 | |
| 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. | |