| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63.80 | 231.44 | 34.53 | 125.00 | -13.25 | 121.54 | -12.61 | 147.82 | 0.3999 | 580.7 | 288.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.76 | 199.63 | 12.24 | 107.50 | -13.20 | 122.37 | -11.78 | 149.36 | 0.3917 | 1386.5 | 360.7 | |
| 13.79 | -1.00 | 7.42 | -1.00 | -13.05 | 122.03 | -12.12 | 148.44 | 0.3924 | 1272.9 | 999999 | |
| 12.48 | -1.00 | 6.73 | -1.00 | -13.44 | 121.98 | -12.17 | 148.85 | 0.3981 | 1086.8 | 999999 | |
| 1.23 | 2.81 | 0.67 | 1.52 | -13.58 | 121.12 | -13.03 | 147.29 | 0.4073 | 782.3 | 631.3 | |
| 1.41 | 3.25 | 0.77 | 1.77 | -13.40 | 119.64 | -14.51 | 144.17 | 0.4182 | 842.3 | 589.8 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -13.12 | 119.50 | -14.65 | 143.50 | 0.4159 | 814.0 | 714.5 | |
| 0.00 | 0.97 | 0.00 | 0.53 | -14.34 | 119.42 | -14.73 | 145.07 | 0.4321 | -464.0 | -455.8 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -13.02 | 117.56 | -16.60 | 139.88 | 0.4337 | -832.0 | -716.0 | |
| 2.46 | 4.31 | 1.36 | 2.37 | -13.35 | 117.34 | -16.81 | 140.01 | 0.4397 | -1053.6 | -822.2 | |
| 0.00 | 2.20 | 0.00 | 1.21 | -13.10 | 117.13 | -17.02 | 139.29 | 0.4389 | -1080.0 | -860.6 | |
| 9.67 | 12.74 | 5.34 | 7.04 | -13.30 | 116.67 | -17.49 | 138.83 | 0.4461 | -1010.9 | -754.6 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -13.71 | 116.15 | -18.00 | 138.61 | 0.4560 | -785.0 | -552.1 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -15.33 | 115.65 | -18.50 | 140.16 | 0.4798 | -836.0 | -763.4 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -14.03 | 115.14 | -19.01 | 137.55 | 0.4701 | -773.0 | -677.9 | |
| 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. | |