| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.65 | 65.03 | 11.22 | 33.67 | -13.10 | 44.33 | -14.55 | 123.03 | 0.2929 | -287.8 | -230.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.93 | 1.78 | 0.48 | 0.91 | -12.72 | 47.17 | -11.71 | 127.34 | 0.2503 | 923.4 | 680.3 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -13.12 | 46.53 | -12.35 | 127.23 | 0.2629 | 729.0 | 510.9 | |
| 0.00 | 2.04 | 0.00 | 1.05 | -13.33 | 46.45 | -12.43 | 127.71 | 0.2659 | 1006.0 | 809.9 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -13.57 | 46.35 | -12.53 | 128.20 | 0.2696 | 843.0 | 697.4 | |
| 0.76 | 1.78 | 0.39 | 0.92 | -13.78 | 46.15 | -12.73 | 128.39 | 0.2743 | 908.1 | 723.3 | |
| 0.00 | 3.40 | 0.00 | 1.74 | -12.67 | 46.15 | -12.73 | 125.00 | 0.2637 | 816.0 | 822.8 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -13.20 | 45.87 | -13.01 | 126.10 | 0.2725 | 857.0 | 702.4 | |
| 0.00 | 0.76 | 0.00 | 0.39 | -12.57 | 45.53 | -13.35 | 123.48 | 0.2714 | 627.0 | 587.1 | |
| 0.00 | 0.93 | 0.00 | 0.48 | -12.68 | 45.09 | -13.79 | 123.01 | 0.2785 | -859.0 | -666.1 | |
| 0.68 | 3.74 | 0.35 | 1.93 | -12.68 | 44.75 | -14.13 | 122.38 | 0.2833 | -1009.4 | -752.8 | |
| 0.00 | 1.78 | 0.00 | 0.92 | -12.44 | 44.73 | -14.15 | 121.62 | 0.2816 | -790.0 | -640.6 | |
| 0.00 | 1.10 | 0.00 | 0.57 | -12.85 | 44.37 | -14.51 | 122.24 | 0.2902 | -1027.0 | -842.2 | |
| 1.53 | 41.62 | 0.79 | 21.60 | -12.96 | 44.20 | -14.68 | 122.32 | 0.2935 | -1174.7 | -610.5 | |
| 0.00 | 1.87 | 0.00 | 0.97 | -13.98 | 43.95 | -14.93 | 124.78 | 0.3058 | 685.0 | 519.0 | |
| 0.51 | -13.00 | 0.26 | -13.00 | -13.55 | 43.82 | -15.06 | 123.39 | 0.3039 | -911.0 | 999999 | |
| 17.24 | -13.00 | 8.95 | -13.00 | -13.10 | 43.69 | -15.19 | 121.89 | 0.3019 | -1076.1 | 999999 | |
| 0.00 | 1.78 | 0.00 | 0.93 | -13.49 | 43.42 | -15.46 | 122.54 | 0.3090 | 8.0 | -8.6 | |
| 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. | |