| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.98 | 258.75 | 29.82 | 173.06 | -23.86 | 193.79 | -37.76 | 123.44 | 0.6728 | 582.2 | 258.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.89 | 243.64 | 1.24 | 161.68 | -23.82 | 194.80 | -36.74 | 123.93 | 0.6619 | 1088.5 | 319.2 | |
| 43.09 | -1.00 | 28.58 | -1.00 | -23.70 | 194.26 | -37.29 | 123.46 | 0.6672 | 1003.4 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.67 | -23.28 | 192.16 | -39.38 | 121.76 | 0.6877 | 504.0 | 403.6 | |
| 0.00 | 0.63 | 0.00 | 0.44 | -23.68 | 191.07 | -40.48 | 121.73 | 0.7013 | -507.0 | -424.6 | |
| 0.00 | 1.17 | 0.00 | 0.86 | -25.79 | 188.07 | -43.48 | 123.05 | 0.7414 | -701.0 | -549.6 | |
| 0.00 | 1.44 | 0.00 | 1.06 | -25.62 | 187.96 | -43.58 | 122.79 | 0.7418 | -626.0 | -509.7 | |
| 0.00 | 2.96 | 0.00 | 2.24 | -26.31 | 186.73 | -44.81 | 123.12 | 0.7566 | -719.0 | -581.6 | |
| 0.00 | 1.17 | 0.00 | 0.88 | -26.04 | 186.53 | -45.01 | 122.70 | 0.7574 | -708.0 | -618.3 | |
| 0.00 | 1.26 | 0.00 | 0.96 | -26.13 | 186.25 | -45.30 | 122.69 | 0.7605 | -462.0 | -396.7 | |
| 0.00 | 1.17 | 0.00 | 0.90 | -26.37 | 185.68 | -45.86 | 122.76 | 0.7668 | -507.0 | -484.5 | |
| 0.00 | 1.17 | 0.00 | 0.89 | -26.04 | 185.76 | -45.79 | 122.38 | 0.7649 | -577.0 | -441.1 | |
| 0.00 | 1.53 | 0.00 | 1.21 | -27.85 | 184.64 | -46.91 | 124.13 | 0.7822 | -588.0 | -526.9 | |
| 0.00 | 0.54 | 0.00 | 0.44 | -29.21 | 183.47 | -48.08 | 125.27 | 0.7977 | -517.0 | -390.3 | |
| 0.00 | 1.08 | 0.00 | 0.83 | -25.29 | 185.06 | -46.48 | 121.18 | 0.7686 | -270.0 | -273.0 | |
| 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. | |