| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.56 | 49.51 | 18.08 | 36.26 | -12.30 | 116.67 | -47.01 | 103.78 | 0.7370 | 412.6 | 16.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.51 | 0.00 | 0.36 | -17.38 | 119.12 | -44.56 | 111.21 | 0.7207 | 429.0 | 491.8 | |
| 0.00 | 1.02 | 0.00 | 0.73 | -15.10 | 118.61 | -45.07 | 107.97 | 0.7210 | 690.0 | 584.7 | |
| 0.00 | 1.10 | 0.00 | 0.78 | -14.48 | 118.78 | -44.90 | 107.15 | 0.7177 | 733.0 | 563.8 | |
| 15.37 | 19.96 | 10.72 | 13.92 | -11.34 | 119.24 | -44.44 | 102.87 | 0.7066 | 851.6 | 542.2 | |
| 9.85 | 14.10 | 7.08 | 10.13 | -12.32 | 117.66 | -46.03 | 103.97 | 0.7269 | 716.0 | 515.0 | |
| 0.00 | 0.59 | 0.00 | 0.42 | -10.30 | 117.95 | -45.73 | 101.23 | 0.7207 | 538.0 | 563.0 | |
| 0.00 | 0.34 | 0.00 | 0.25 | -12.99 | 115.49 | -48.19 | 104.49 | 0.7526 | -445.0 | -391.2 | |
| 0.00 | 1.19 | 0.00 | 0.90 | -12.43 | 115.13 | -48.55 | 103.70 | 0.7558 | -633.0 | -542.8 | |
| 0.00 | 0.42 | 0.00 | 0.35 | -13.51 | 111.58 | -52.10 | 104.58 | 0.7951 | -614.0 | -547.8 | |
| 0.00 | 1.19 | 0.00 | 0.96 | -12.79 | 111.75 | -51.93 | 103.71 | 0.7925 | -610.0 | -491.4 | |
| 0.34 | 4.33 | 0.28 | 3.54 | -14.01 | 111.27 | -52.41 | 105.16 | 0.7988 | -666.2 | -468.5 | |
| 0.00 | 3.57 | 0.00 | 2.89 | -12.39 | 111.52 | -52.16 | 103.17 | 0.7945 | -344.0 | -393.3 | |
| 0.00 | 0.51 | 0.00 | 0.42 | -13.37 | 111.18 | -52.50 | 104.35 | 0.7990 | -364.0 | -409.2 | |
| 0.00 | 0.68 | 0.00 | 0.61 | -13.01 | 107.20 | -56.48 | 103.46 | 0.8374 | -313.0 | -323.0 | |
| 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. | |