| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.35 | 0.00 | 9.00 | -21.01 | 320.71 | 27.42 | 234.98 | 0.5231 | -106.6 | 27.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.62 | 0.00 | 0.41 | -15.52 | 333.86 | 40.57 | 252.96 | 0.6577 | 512.0 | 392.1 | |
| 0.00 | 1.41 | 0.00 | 0.91 | -16.86 | 332.63 | 39.34 | 250.60 | 0.6455 | 696.0 | 562.6 | |
| 0.00 | 0.79 | 0.00 | 0.51 | -16.84 | 331.49 | 38.20 | 250.30 | 0.6310 | 617.0 | 542.1 | |
| 0.00 | 1.50 | 0.00 | 0.92 | -18.33 | 327.99 | 34.70 | 246.59 | 0.5911 | 676.0 | 521.5 | |
| 0.00 | 1.59 | 0.00 | 0.95 | -19.70 | 325.14 | 31.85 | 242.89 | 0.5602 | 836.0 | 675.9 | |
| 0.00 | 1.85 | 0.00 | 1.10 | -19.52 | 324.91 | 31.62 | 243.06 | 0.5565 | 550.0 | 417.1 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -20.89 | 318.72 | 25.43 | 236.12 | 0.4852 | -321.0 | -218.4 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -23.98 | 317.15 | 23.86 | 229.14 | 0.4907 | -719.0 | -646.3 | |
| 0.00 | 0.35 | 0.00 | 0.20 | -22.21 | 316.22 | 22.93 | 231.23 | 0.4646 | -579.0 | -571.5 | |
| 0.00 | 0.62 | 0.00 | 0.35 | -25.10 | 314.39 | 21.10 | 224.11 | 0.4704 | -726.0 | -580.7 | |
| 0.00 | 1.59 | 0.00 | 0.87 | -23.83 | 311.21 | 17.92 | 221.89 | 0.4233 | -715.0 | -580.3 | |
| 0.00 | 1.24 | 0.00 | 0.68 | -25.10 | 309.80 | 16.51 | 217.60 | 0.4235 | -750.0 | -541.6 | |
| 0.00 | 1.24 | 0.00 | 0.67 | -25.55 | 307.06 | 13.77 | 212.25 | 0.4042 | -746.0 | -527.6 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -25.43 | 306.81 | 13.52 | 211.97 | 0.4005 | -824.0 | -681.1 | |
| 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. | |