| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.12 | 131.34 | 35.99 | 98.64 | 7.05 | 210.14 | 49.05 | 273.54 | 0.7528 | -30.0 | -19.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.21 | 36.07 | 5.69 | 28.41 | 7.49 | 212.58 | 51.49 | 274.27 | 0.7802 | -704.4 | -305.0 | |
| 0.00 | 0.35 | 0.00 | 0.27 | 6.83 | 211.85 | 50.75 | 273.38 | 0.7726 | -200.0 | -200.2 | |
| 14.87 | 23.14 | 11.53 | 17.91 | 7.20 | 211.76 | 50.67 | 273.85 | 0.7714 | -818.7 | -582.0 | |
| 0.00 | 2.20 | 0.00 | 1.70 | 9.49 | 211.84 | 50.75 | 276.83 | 0.7715 | -208.0 | -304.4 | |
| 0.00 | 1.50 | 0.00 | 1.14 | 7.35 | 211.12 | 50.02 | 274.01 | 0.7642 | -251.0 | -267.2 | |
| 0.00 | 1.58 | 0.00 | 1.19 | 6.16 | 210.20 | 49.11 | 272.38 | 0.7545 | -656.0 | -617.7 | |
| 0.00 | 0.35 | 0.00 | 0.26 | 6.77 | 209.13 | 48.04 | 273.11 | 0.7418 | 168.0 | 142.0 | |
| 0.79 | 26.65 | 0.58 | 19.44 | 6.34 | 208.81 | 47.71 | 272.51 | 0.7383 | 413.2 | 167.7 | |
| 2.20 | -8.00 | 1.60 | -8.00 | 6.81 | 208.60 | 47.50 | 273.14 | 0.7355 | -262.0 | 999999 | |
| 7.74 | -8.00 | 5.63 | -8.00 | 6.46 | 208.51 | 47.41 | 272.65 | 0.7347 | 704.5 | 999999 | |
| 0.97 | 34.57 | 0.70 | 24.83 | 6.48 | 207.93 | 46.83 | 272.63 | 0.7278 | 636.5 | 517.9 | |
| 13.28 | -11.00 | 9.51 | -11.00 | 6.77 | 207.66 | 46.56 | 273.02 | 0.7244 | 836.2 | 999999 | |
| 0.00 | 2.20 | 0.00 | 1.57 | 6.14 | 207.58 | 46.49 | 272.15 | 0.7239 | 617.0 | 503.4 | |
| 1.06 | 2.73 | 0.75 | 1.92 | 7.20 | 206.88 | 45.78 | 273.57 | 0.7148 | 710.7 | 571.8 | |
| 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. | |