| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.68 | 115.82 | 24.25 | 58.96 | 12.68 | 114.94 | -10.44 | 50.17 | 0.2311 | -557.0 | -73.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.38 | 0.00 | 0.70 | 11.87 | 115.95 | -9.43 | 50.53 | 0.2087 | 161.0 | 176.1 | |
| 35.82 | 77.86 | 18.19 | 39.56 | 12.79 | 115.70 | -9.68 | 47.90 | 0.2221 | -1225.7 | -359.2 | |
| 3.55 | -2.00 | 1.81 | -2.00 | 13.06 | 115.04 | -10.34 | 48.85 | 0.2334 | -519.6 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.70 | 11.76 | 115.06 | -10.32 | 53.35 | 0.2197 | -774.0 | -410.7 | |
| 1.99 | 3.46 | 1.02 | 1.77 | 13.23 | 114.54 | -10.85 | 49.59 | 0.2417 | -920.7 | -661.4 | |
| 2.16 | 11.68 | 1.10 | 5.94 | 11.90 | 114.06 | -11.32 | 55.26 | 0.2348 | 1018.9 | -55.4 | |
| 0.00 | 1.12 | 0.00 | 0.57 | 12.08 | 113.81 | -11.58 | 55.22 | 0.2400 | 877.0 | 629.3 | |
| 2.34 | 3.81 | 1.20 | 1.95 | 13.28 | 113.41 | -11.97 | 52.12 | 0.2570 | -777.6 | -526.1 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 11.86 | 113.45 | -11.94 | 56.76 | 0.2431 | 1023.0 | 780.5 | |
| 1.82 | 5.19 | 0.93 | 2.66 | 12.70 | 112.88 | -12.51 | 55.13 | 0.2587 | 1178.9 | 928.3 | |
| 0.00 | 3.98 | 0.00 | 2.04 | 12.66 | 112.54 | -12.85 | 55.93 | 0.2631 | 800.0 | 729.6 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 12.24 | 112.53 | -12.86 | 57.34 | 0.2595 | 875.0 | 630.3 | |
| 0.00 | 2.42 | 0.00 | 1.25 | 12.83 | 111.49 | -13.89 | 57.38 | 0.2792 | 1159.0 | 909.7 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 11.83 | 111.55 | -13.84 | 60.45 | 0.2703 | 807.0 | 561.3 | |
| 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. | |