| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.59 | 36.97 | 6.06 | 19.35 | -15.78 | 244.86 | -9.01 | 152.61 | 0.3257 | -155.6 | -80.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.65 | -13.87 | 251.97 | -1.90 | 172.78 | 0.2566 | 821.0 | 633.6 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -16.66 | 249.72 | -4.15 | 167.00 | 0.3094 | 694.0 | 631.2 | |
| 0.00 | 2.81 | 0.00 | 1.46 | -15.48 | 247.53 | -6.34 | 159.22 | 0.3014 | 903.0 | 708.6 | |
| 5.34 | 6.79 | 2.77 | 3.52 | -14.66 | 246.66 | -7.21 | 155.54 | 0.2943 | 1054.7 | 900.6 | |
| 0.00 | 3.26 | 0.00 | 1.69 | -14.79 | 245.77 | -8.10 | 153.13 | 0.3027 | 815.0 | 686.6 | |
| 0.00 | 1.81 | 0.00 | 0.97 | -19.31 | 243.81 | -10.06 | 154.37 | 0.3829 | 688.0 | 430.9 | |
| 0.00 | 1.72 | 0.00 | 0.90 | -16.03 | 243.80 | -10.07 | 149.87 | 0.3363 | -956.0 | -797.6 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -16.10 | 243.57 | -10.30 | 149.41 | 0.3391 | -861.0 | -727.9 | |
| 6.25 | 8.70 | 3.29 | 4.57 | -15.78 | 243.26 | -10.61 | 148.17 | 0.3373 | -1110.2 | -822.6 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -16.67 | 243.15 | -10.72 | 149.31 | 0.3506 | -767.0 | -656.8 | |
| 0.00 | 1.90 | 0.00 | 1.00 | -16.16 | 242.82 | -11.05 | 147.75 | 0.3464 | -835.0 | -719.9 | |
| 0.00 | 2.45 | 0.00 | 1.29 | -15.81 | 242.59 | -11.29 | 146.63 | 0.3438 | -956.0 | -788.0 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -16.74 | 242.17 | -11.70 | 147.20 | 0.3600 | -740.0 | -603.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -17.76 | 241.52 | -12.35 | 147.38 | 0.3795 | -886.0 | -750.3 | |
| 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. | |