| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.21 | 28.26 | 1.16 | 14.94 | -19.77 | 322.82 | -7.39 | 159.48 | 0.3466 | -435.0 | -302.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.62 | 0.00 | 0.86 | -21.65 | 327.24 | -2.97 | 172.24 | 0.3583 | -897.0 | -776.5 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -16.98 | 326.45 | -3.75 | 167.24 | 0.2845 | 963.0 | 701.8 | |
| 0.00 | 4.51 | 0.00 | 2.35 | -18.06 | 324.63 | -5.58 | 162.57 | 0.3098 | 1046.0 | 825.2 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -17.75 | 324.64 | -5.57 | 162.28 | 0.3049 | 956.0 | 717.3 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -23.68 | 323.96 | -6.25 | 165.54 | 0.4008 | -773.0 | -665.8 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -16.82 | 323.36 | -6.84 | 157.38 | 0.2978 | -961.0 | -649.2 | |
| 0.00 | 1.87 | 0.00 | 0.97 | -16.95 | 323.02 | -7.19 | 156.54 | 0.3020 | -910.0 | -631.7 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -28.00 | 322.07 | -8.13 | 164.65 | 0.4738 | -436.0 | -455.9 | |
| 2.21 | 3.91 | 1.16 | 2.05 | -18.02 | 322.47 | -7.73 | 156.47 | 0.3219 | -1014.6 | -816.2 | |
| 0.00 | 3.06 | 0.00 | 1.60 | -17.53 | 322.15 | -8.05 | 154.93 | 0.3167 | -1071.0 | -873.8 | |
| 0.00 | 3.91 | 0.00 | 2.05 | -17.99 | 322.07 | -8.14 | 155.34 | 0.3241 | -709.0 | -605.6 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -24.09 | 320.51 | -9.69 | 158.65 | 0.4240 | -782.0 | -677.2 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -23.54 | 319.41 | -10.79 | 155.93 | 0.4228 | -720.0 | -628.3 | |
| 0.00 | 2.13 | 0.00 | 1.20 | -27.50 | 318.30 | -11.91 | 157.74 | 0.4853 | -689.0 | -497.0 | |
| 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. | |