| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.11 | 0.00 | 9.75 | 4.16 | 260.05 | -20.57 | 75.13 | 0.3587 | -40.0 | 62.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.68 | 5.95 | 273.86 | -6.76 | 48.50 | 0.1571 | -875.0 | -708.1 | |
| 0.00 | 0.81 | 0.00 | 0.41 | 5.03 | 273.68 | -6.94 | 53.91 | 0.1495 | -990.0 | -752.4 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 5.64 | 271.80 | -8.82 | 57.21 | 0.1824 | -806.0 | -670.8 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 2.17 | 270.07 | -10.55 | 78.30 | 0.1877 | -834.0 | -574.2 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 2.20 | 269.94 | -10.68 | 78.28 | 0.1899 | -844.0 | -683.7 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 1.68 | 269.14 | -11.48 | 81.59 | 0.2020 | -859.0 | -637.8 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 1.41 | 267.77 | -12.85 | 83.67 | 0.2246 | -963.0 | -699.1 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 8.42 | 259.99 | -20.63 | 67.22 | 0.3796 | 631.0 | 407.0 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 5.81 | 259.52 | -21.10 | 74.21 | 0.3738 | 879.0 | 674.1 | |
| 0.00 | 1.72 | 0.00 | 0.94 | 5.79 | 256.20 | -24.42 | 76.23 | 0.4252 | 703.0 | 570.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 1.37 | 254.57 | -26.05 | 86.89 | 0.4414 | 771.0 | 650.9 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 4.29 | 254.10 | -26.52 | 80.46 | 0.4534 | 810.0 | 673.9 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 6.19 | 251.55 | -29.07 | 77.42 | 0.4968 | 631.0 | 564.8 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 9.42 | 248.91 | -31.71 | 72.49 | 0.5459 | 689.0 | 555.5 | |
| 0.00 | 1.54 | 0.00 | 0.98 | -0.41 | 241.69 | -38.93 | 90.66 | 0.6306 | 457.0 | 385.6 | |
| 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. | |