| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.90 | 358.90 | 46.95 | 269.66 | 11.92 | 262.07 | 45.15 | 292.73 | 0.7534 | -576.8 | -286.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.90 | 342.61 | 46.95 | 259.61 | 11.91 | 262.62 | 45.70 | 292.36 | 0.7595 | -876.0 | -319.9 | |
| 0.00 | 0.78 | 0.00 | 0.57 | 13.16 | 259.68 | 42.76 | 295.35 | 0.7338 | -657.0 | -531.0 | |
| 0.00 | 1.48 | 0.00 | 0.92 | 11.31 | 249.45 | 32.53 | 299.26 | 0.6066 | 587.0 | 485.2 | |
| 0.00 | 1.83 | 0.00 | 1.13 | 11.27 | 248.94 | 32.02 | 299.60 | 0.6002 | 193.0 | 247.1 | |
| 0.00 | 0.87 | 0.00 | 0.55 | 12.83 | 249.11 | 32.19 | 301.71 | 0.6129 | 619.0 | 499.6 | |
| 0.00 | 0.78 | 0.00 | 0.49 | 11.86 | 248.87 | 31.95 | 300.52 | 0.6034 | 622.0 | 482.1 | |
| 0.00 | 0.78 | 0.00 | 0.48 | 11.41 | 248.63 | 31.71 | 300.05 | 0.5975 | 770.0 | 618.8 | |
| 0.00 | 0.87 | 0.00 | 0.54 | 11.80 | 248.32 | 31.40 | 300.86 | 0.5964 | 744.0 | 689.7 | |
| 0.00 | 3.31 | 0.00 | 2.05 | 12.65 | 248.29 | 31.37 | 302.12 | 0.6020 | 563.0 | 490.8 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 11.37 | 247.06 | 30.14 | 301.28 | 0.5782 | 753.0 | 580.4 | |
| 0.00 | 1.31 | 0.00 | 0.79 | 13.48 | 245.96 | 29.04 | 305.37 | 0.5810 | 569.0 | 439.9 | |
| 0.00 | 0.70 | 0.00 | 0.41 | 10.54 | 243.58 | 26.66 | 303.20 | 0.5293 | 503.0 | 418.0 | |
| 0.00 | 1.05 | 0.00 | 0.62 | 14.90 | 242.81 | 25.89 | 310.56 | 0.5576 | 568.0 | 524.0 | |
| 0.00 | 1.48 | 0.00 | 0.87 | 12.73 | 242.21 | 25.29 | 308.06 | 0.5313 | 713.0 | 556.5 | |
| 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. | |