| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 192 | 1220 | 128 | 825 | 10.22 | 309.19 | -41.55 | 74.83 | 0.6732 | 731.1 | 76.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | 14.09 | 300.71 | -50.02 | 72.04 | 0.7836 | -186.0 | -173.4 | |
| 74 | 691 | 46 | 424 | 9.71 | 315.83 | -34.90 | 73.66 | 0.5900 | 1899.7 | 595.7 | |
| 5 | -2 | 3 | -2 | 9.66 | 315.05 | -35.68 | 74.03 | 0.6004 | 991.3 | 999999 | |
| 3 | 18 | 2 | 11 | 10.24 | 312.38 | -38.35 | 74.04 | 0.6374 | 732.0 | 540.4 | |
| 3 | -2 | 2 | -2 | 9.65 | 314.28 | -36.46 | 74.32 | 0.6108 | 495.2 | 999999 | |
| 23 | -2 | 14 | -2 | 9.31 | 315.03 | -35.71 | 74.61 | 0.5996 | 1243.4 | 999999 | |
| 2 | -4 | 2 | -4 | 9.98 | 312.18 | -38.55 | 74.51 | 0.6393 | 710.7 | 999999 | |
| 23 | -2 | 14 | -2 | 8.94 | 315.46 | -35.27 | 75.07 | 0.5927 | 1827.0 | 999999 | |
| 6 | 13 | 4 | 9 | 9.68 | 312.66 | -38.07 | 74.82 | 0.6322 | 895.6 | 600.5 | |
| 0 | 7 | 0 | 4 | 9.09 | 312.19 | -38.54 | 75.87 | 0.6368 | 777.0 | 748.6 | |
| 2 | 7 | 2 | 5 | 10.06 | 308.26 | -42.47 | 75.52 | 0.6890 | 438.2 | 226.9 | |
| 0 | 5 | 0 | 4 | 11.22 | 303.36 | -47.37 | 75.11 | 0.7492 | -757.0 | -670.4 | |
| 0 | 6 | 0 | 4 | 8.75 | 312.28 | -38.46 | 76.38 | 0.6348 | 773.0 | 540.5 | |
| 5 | 435 | 4 | 335 | 11.25 | 302.43 | -48.30 | 75.28 | 0.7595 | -1320.7 | -525.6 | |
| 18 | -14 | 13 | -14 | 11.20 | 301.97 | -48.76 | 75.44 | 0.7645 | -1249.7 | 999999 | |
| 28 | -14 | 22 | -14 | 11.20 | 301.27 | -49.46 | 75.58 | 0.7721 | -886.5 | 999999 | |
| 0 | 6 | 0 | 5 | 9.55 | 304.22 | -46.51 | 77.16 | 0.7362 | -781.0 | -629.2 | |
| 0 | 13 | 0 | 10 | 9.94 | 300.22 | -50.52 | 77.39 | 0.7814 | -254.0 | 91.7 | |
| 0 | 10 | 0 | 8 | 9.44 | 301.38 | -49.35 | 77.84 | 0.7680 | -470.0 | -462.8 | |
| 0 | 6 | 0 | 4 | 9.56 | 300.66 | -50.08 | 77.80 | 0.7761 | -313.0 | -310.4 | |
| 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. | |