| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.59 | 158.46 | 21.09 | 100.22 | 6.60 | 203.43 | -38.43 | 83.77 | 0.6231 | -590.6 | -328.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.90 | 12.62 | 2.42 | 7.84 | 6.96 | 204.79 | -37.08 | 83.07 | 0.6051 | -1076.5 | -661.8 | |
| 3.72 | -1.00 | 2.32 | -1.00 | 7.11 | 204.70 | -37.17 | 82.83 | 0.6064 | -876.6 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.51 | 3.69 | 204.94 | -36.93 | 88.49 | 0.6020 | -550.0 | -424.8 | |
| 24.24 | 127.39 | 15.25 | 80.10 | 6.46 | 203.82 | -38.04 | 83.96 | 0.6180 | -1199.8 | -387.1 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 8.58 | 203.21 | -38.65 | 80.62 | 0.6282 | -681.0 | -602.1 | |
| 0.82 | 3.00 | 0.52 | 1.90 | 7.42 | 203.14 | -38.72 | 82.49 | 0.6279 | -750.8 | -547.1 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 8.02 | 202.88 | -38.99 | 81.56 | 0.6320 | -460.0 | -418.5 | |
| 0.91 | 3.18 | 0.58 | 2.03 | 7.37 | 202.79 | -39.07 | 82.59 | 0.6326 | -525.5 | -438.4 | |
| 0.00 | 1.09 | 0.00 | 0.73 | 5.84 | 199.53 | -42.33 | 85.15 | 0.6747 | 752.0 | 634.2 | |
| 0.00 | 1.27 | 0.00 | 0.86 | 6.84 | 199.22 | -42.64 | 83.69 | 0.6790 | 607.0 | 491.8 | |
| 0.00 | 0.64 | 0.00 | 0.44 | 7.95 | 197.21 | -44.66 | 82.21 | 0.7049 | 710.0 | 661.4 | |
| 0.00 | 0.54 | 0.00 | 0.38 | 7.68 | 197.20 | -44.66 | 82.60 | 0.7048 | 657.0 | 558.0 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 7.51 | 197.01 | -44.86 | 82.85 | 0.7071 | 611.0 | 564.7 | |
| 0.00 | 1.91 | 0.00 | 1.34 | 8.21 | 196.87 | -45.00 | 81.87 | 0.7092 | 726.0 | 556.3 | |
| 0.00 | 1.09 | 0.00 | 0.76 | 6.59 | 196.95 | -44.92 | 84.16 | 0.7074 | 745.0 | 584.1 | |
| 0.00 | 1.73 | 0.00 | 1.21 | 6.80 | 196.79 | -45.07 | 83.87 | 0.7094 | 634.0 | 455.4 | |
| 0.00 | 1.09 | 0.00 | 0.77 | 7.25 | 196.56 | -45.31 | 83.25 | 0.7124 | 335.0 | 231.7 | |
| 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. | |