| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.45 | 112.01 | 18.50 | 101.13 | -14.68 | 119.21 | 53.31 | 248.08 | 0.8378 | 147.0 | 216.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.01 | 94.63 | 1.84 | 86.89 | -13.97 | 120.03 | 54.13 | 249.20 | 0.8433 | 598.8 | 331.9 | |
| 0.00 | 0.61 | 0.00 | 0.53 | -10.63 | 119.03 | 53.13 | 252.73 | 0.8255 | 399.0 | 332.7 | |
| 16.08 | -1.00 | 14.79 | -1.00 | -14.66 | 119.95 | 54.05 | 248.39 | 0.8445 | 757.3 | 999999 | |
| 0.00 | 0.61 | 0.00 | 0.56 | -17.77 | 118.97 | 53.07 | 244.54 | 0.8453 | -283.0 | -272.3 | |
| 0.00 | 0.70 | 0.00 | 0.59 | -16.20 | 116.03 | 50.13 | 245.17 | 0.8143 | -554.0 | -425.1 | |
| 0.00 | 0.87 | 0.00 | 0.73 | -15.99 | 115.43 | 49.53 | 245.17 | 0.8080 | -481.0 | -423.4 | |
| 0.00 | 0.52 | 0.00 | 0.44 | -16.21 | 115.31 | 49.41 | 244.87 | 0.8077 | -268.0 | -324.0 | |
| 0.00 | 1.22 | 0.00 | 1.02 | -16.12 | 115.09 | 49.19 | 244.87 | 0.8053 | -587.0 | -542.0 | |
| 0.00 | 1.14 | 0.00 | 0.95 | -16.38 | 115.08 | 49.18 | 244.57 | 0.8062 | -504.0 | -453.1 | |
| 0.00 | 1.83 | 0.00 | 1.48 | -14.35 | 114.39 | 48.49 | 246.68 | 0.7923 | -649.0 | -517.0 | |
| 0.00 | 0.70 | 0.00 | 0.59 | -16.77 | 115.17 | 49.27 | 244.15 | 0.8084 | -309.0 | -237.8 | |
| 0.00 | 0.96 | 0.00 | 0.78 | -14.63 | 114.28 | 48.38 | 246.31 | 0.7922 | -583.0 | -458.6 | |
| 0.00 | 1.31 | 0.00 | 1.08 | -16.42 | 114.76 | 48.86 | 244.39 | 0.8033 | -727.0 | -651.3 | |
| 0.00 | 1.66 | 0.00 | 1.35 | -16.17 | 114.01 | 48.11 | 244.37 | 0.7953 | -657.0 | -478.3 | |
| 2.36 | 4.11 | 1.87 | 3.25 | -14.30 | 113.40 | 47.50 | 246.32 | 0.7824 | -616.4 | -498.6 | |
| 0.00 | 0.70 | 0.00 | 0.55 | -14.42 | 112.84 | 46.94 | 245.95 | 0.7772 | -573.0 | -500.8 | |
| 0.00 | 0.44 | 0.00 | 0.34 | -15.55 | 111.41 | 45.51 | 243.93 | 0.7674 | -595.0 | -563.0 | |
| 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. | |