| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.81 | 0.00 | 10.85 | -14.90 | 36.40 | 9.07 | 209.40 | 0.3042 | -453.1 | -417.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.79 | 0.00 | 0.99 | -20.90 | 43.44 | 16.11 | 215.76 | 0.4455 | -901.0 | -716.8 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -17.51 | 41.11 | 13.79 | 216.77 | 0.3814 | 715.0 | 492.4 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -15.26 | 38.91 | 11.59 | 216.03 | 0.3310 | 948.0 | 777.8 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -15.13 | 37.75 | 10.43 | 213.46 | 0.3184 | 806.0 | 717.9 | |
| 0.00 | 0.77 | 0.00 | 0.40 | -13.21 | 36.81 | 9.48 | 214.66 | 0.2833 | -702.0 | -524.3 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -12.63 | 36.26 | 8.94 | 214.32 | 0.2702 | -717.0 | -651.8 | |
| 0.00 | 1.79 | 0.00 | 0.92 | -13.09 | 35.85 | 8.52 | 212.14 | 0.2727 | -895.0 | -726.8 | |
| 0.00 | 2.39 | 0.00 | 1.24 | -14.49 | 35.44 | 8.11 | 208.32 | 0.2893 | -1029.0 | -856.9 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -15.71 | 35.24 | 7.91 | 205.79 | 0.3059 | -765.0 | -705.6 | |
| 0.00 | 1.71 | 0.00 | 0.88 | -14.49 | 35.19 | 7.87 | 207.59 | 0.2874 | -993.0 | -729.7 | |
| 0.00 | 0.43 | 0.00 | 0.22 | -15.01 | 34.96 | 7.64 | 206.08 | 0.2934 | -556.0 | -629.2 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -14.67 | 34.92 | 7.60 | 206.49 | 0.2880 | -816.0 | -767.9 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -12.48 | 34.33 | 7.01 | 208.49 | 0.2509 | -836.0 | -685.9 | |
| 0.00 | 2.64 | 0.00 | 1.35 | -13.08 | 31.15 | 3.83 | 195.80 | 0.2399 | -602.0 | -558.0 | |
| 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. | |