| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.99 | 35.88 | 8.66 | 24.97 | -16.14 | 232.80 | -40.53 | 117.09 | 0.7023 | -120.1 | 14.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.70 | -17.51 | 239.79 | -33.53 | 123.23 | 0.6321 | 330.0 | 300.5 | |
| 1.09 | 3.09 | 0.71 | 2.01 | -14.21 | 236.42 | -36.91 | 116.38 | 0.6521 | 782.1 | 603.0 | |
| 0.00 | 0.82 | 0.00 | 0.53 | -14.37 | 236.23 | -37.10 | 116.50 | 0.6552 | 351.0 | 321.7 | |
| 0.00 | 1.09 | 0.00 | 0.72 | -15.22 | 235.78 | -37.55 | 117.43 | 0.6648 | 443.0 | 414.0 | |
| 0.00 | 1.18 | 0.00 | 0.78 | -14.35 | 235.88 | -37.45 | 116.28 | 0.6593 | 682.0 | 636.5 | |
| 0.00 | 0.82 | 0.00 | 0.55 | -15.94 | 235.50 | -37.83 | 118.26 | 0.6718 | 507.0 | 383.6 | |
| 0.00 | 1.09 | 0.00 | 0.73 | -15.21 | 235.26 | -38.07 | 117.12 | 0.6708 | 612.0 | 518.8 | |
| 0.00 | 2.09 | 0.00 | 1.39 | -14.72 | 235.32 | -38.01 | 116.48 | 0.6676 | 811.0 | 654.3 | |
| 0.00 | 1.54 | 0.00 | 1.03 | -14.95 | 235.19 | -38.13 | 116.73 | 0.6703 | 469.0 | 374.8 | |
| 0.00 | 1.00 | 0.00 | 0.68 | -15.57 | 234.00 | -39.33 | 116.92 | 0.6870 | -605.0 | -478.2 | |
| 0.64 | 1.63 | 0.43 | 1.10 | -14.41 | 234.22 | -39.11 | 115.46 | 0.6790 | 559.4 | 449.1 | |
| 0.00 | 1.00 | 0.00 | 0.68 | -15.35 | 233.85 | -39.48 | 116.54 | 0.6877 | -581.0 | -458.1 | |
| 0.00 | 1.18 | 0.00 | 0.81 | -14.92 | 233.41 | -39.92 | 115.73 | 0.6906 | -575.0 | -556.5 | |
| 0.00 | 2.36 | 0.00 | 1.64 | -16.35 | 232.90 | -40.43 | 117.38 | 0.7031 | -617.0 | -513.1 | |
| 0.00 | 0.91 | 0.00 | 0.63 | -15.98 | 232.66 | -40.67 | 116.76 | 0.7039 | -637.0 | -465.3 | |
| 6.99 | 14.99 | 5.13 | 10.99 | -17.47 | 229.93 | -43.40 | 117.34 | 0.7401 | -688.2 | -484.2 | |
| 3.27 | -16.00 | 2.39 | -16.00 | -17.14 | 229.98 | -43.35 | 116.95 | 0.7381 | -726.7 | 999999 | |
| 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. | |