| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.14 | 90.69 | 15.00 | 46.56 | 7.90 | 42.99 | -12.87 | 57.32 | 0.2627 | 345.1 | -47.5 | |
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back to the solar disc SDO HMI 2011-12-09 08:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.61 | 33.41 | 4.38 | 17.02 | 7.66 | 45.10 | -10.77 | 53.76 | 0.2306 | -1105.3 | -916.0 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 8.20 | 44.81 | -11.05 | 52.63 | 0.2399 | -1030.0 | -806.3 | |
| 0.00 | 3.67 | 0.00 | 1.87 | 8.14 | 44.17 | -11.69 | 54.34 | 0.2480 | -924.0 | -600.4 | |
| 0.00 | 1.02 | 0.00 | 0.52 | 7.51 | 44.19 | -11.67 | 56.43 | 0.2418 | -656.0 | -416.8 | |
| 0.00 | 4.94 | 0.00 | 2.54 | 8.44 | 42.70 | -13.17 | 56.51 | 0.2714 | 748.0 | 839.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 8.44 | 42.27 | -13.60 | 57.34 | 0.2775 | 964.0 | 740.0 | |
| 2.13 | 3.92 | 1.10 | 2.02 | 8.17 | 42.22 | -13.65 | 58.27 | 0.2759 | 969.0 | 704.4 | |
| 0.00 | 2.56 | 0.00 | 1.32 | 7.96 | 42.04 | -13.83 | 59.24 | 0.2767 | 741.0 | 584.6 | |
| 0.00 | 2.47 | 0.00 | 1.27 | 7.42 | 41.87 | -13.99 | 61.24 | 0.2747 | 987.0 | 692.5 | |
| 1.70 | 36.65 | 0.88 | 18.95 | 7.87 | 41.67 | -14.19 | 60.16 | 0.2812 | 1094.7 | 736.8 | |
| 0.94 | -10.00 | 0.48 | -10.00 | 8.02 | 41.48 | -14.38 | 60.02 | 0.2852 | 1024.9 | 999999 | |
| 3.32 | -10.00 | 1.72 | -10.00 | 7.84 | 41.37 | -14.50 | 60.77 | 0.2855 | 1162.1 | 999999 | |
| 8.86 | -10.00 | 4.59 | -10.00 | 8.08 | 41.11 | -14.75 | 60.46 | 0.2911 | 1047.9 | 999999 | |
| 3.58 | -10.00 | 1.85 | -10.00 | 8.02 | 40.84 | -15.03 | 61.08 | 0.2947 | 861.2 | 999999 | |
| 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. | |