| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.63 | 153.62 | 31.67 | 199.13 | -13.59 | 230.19 | -67.48 | 103.34 | 0.9196 | 362.5 | 118.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 1.10 | -10.12 | 239.29 | -58.37 | 99.86 | 0.8528 | 549.0 | 478.5 | |
| 16.39 | 104.62 | 17.56 | 112.77 | -11.63 | 235.11 | -62.55 | 101.40 | 0.8886 | 808.3 | 253.2 | |
| 1.43 | -2.00 | 1.56 | -2.00 | -11.24 | 234.59 | -63.07 | 100.93 | 0.8925 | 404.4 | 999999 | |
| 0.00 | 1.43 | 0.00 | 1.74 | -10.83 | 231.56 | -66.10 | 100.39 | 0.9147 | 110.0 | 65.6 | |
| 0.00 | 0.63 | 0.00 | 1.06 | -19.52 | 224.45 | -73.21 | 109.41 | 0.9580 | -121.0 | -136.1 | |
| 0.00 | 2.06 | 0.00 | 3.38 | -15.68 | 224.98 | -72.69 | 105.40 | 0.9547 | -61.0 | -105.5 | |
| 6.81 | 33.23 | 12.55 | 61.57 | -17.05 | 223.00 | -74.66 | 106.79 | 0.9642 | 170.0 | 28.1 | |
| 0.00 | 2.24 | 0.00 | 3.63 | -14.81 | 225.21 | -72.45 | 104.50 | 0.9535 | -383.0 | -390.7 | |
| 0.00 | 1.70 | 0.00 | 2.83 | -15.19 | 224.77 | -72.90 | 104.89 | 0.9557 | -436.0 | -414.0 | |
| 0.00 | 0.81 | 0.00 | 1.36 | -15.55 | 224.44 | -73.23 | 105.26 | 0.9574 | -56.0 | -75.2 | |
| 0.00 | 0.27 | 0.00 | 0.46 | -15.02 | 224.38 | -73.28 | 104.70 | 0.9576 | -121.0 | -149.3 | |
| 0.00 | 0.81 | 0.00 | 1.29 | -13.76 | 225.44 | -72.23 | 103.40 | 0.9522 | -182.0 | -262.1 | |
| 0.00 | 2.06 | 0.00 | 3.13 | -11.15 | 226.42 | -71.25 | 100.66 | 0.9468 | -316.0 | -270.7 | |
| 0.00 | 2.60 | 0.00 | 4.81 | -14.12 | 222.89 | -74.77 | 103.74 | 0.9645 | -472.0 | -293.3 | |
| 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. | |