| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.73 | 83.45 | 20.50 | 43.06 | 7.80 | 42.86 | -14.09 | 60.03 | 0.2793 | 144.5 | 59.3 | |
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back to the solar disc SDO HMI 2011-12-09 06:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.65 | 34.10 | 3.40 | 17.45 | 7.67 | 44.94 | -12.01 | 56.66 | 0.2480 | -1145.2 | -837.6 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 8.21 | 44.74 | -12.21 | 55.30 | 0.2558 | -1111.0 | -856.9 | |
| 7.33 | -1.00 | 3.75 | -1.00 | 7.34 | 44.43 | -12.52 | 58.84 | 0.2524 | -1024.4 | 999999 | |
| 3.58 | -1.00 | 1.83 | -1.00 | 7.73 | 44.36 | -12.59 | 57.67 | 0.2568 | -913.5 | 999999 | |
| 0.00 | 1.70 | 0.00 | 0.88 | 8.09 | 44.11 | -12.85 | 57.01 | 0.2637 | -862.0 | -675.4 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 7.58 | 43.17 | -13.78 | 60.40 | 0.2728 | -646.0 | -585.2 | |
| 0.00 | 3.15 | 0.00 | 1.63 | 8.36 | 42.68 | -14.27 | 58.83 | 0.2863 | 919.0 | 820.8 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 7.20 | 42.39 | -14.57 | 62.94 | 0.2815 | 912.0 | 637.3 | |
| 2.05 | 4.94 | 1.06 | 2.56 | 8.15 | 42.23 | -14.72 | 60.23 | 0.2912 | 1103.0 | 872.3 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 7.43 | 41.92 | -15.04 | 62.91 | 0.2903 | 1028.0 | 871.4 | |
| 0.34 | 14.92 | 0.18 | 7.74 | 8.03 | 41.52 | -15.43 | 61.70 | 0.3006 | 1136.8 | 909.3 | |
| 4.86 | -11.00 | 2.52 | -11.00 | 7.79 | 41.47 | -15.48 | 62.49 | 0.2995 | 1058.7 | 999999 | |
| 10.06 | 20.80 | 5.23 | 10.82 | 8.06 | 41.15 | -15.80 | 62.16 | 0.3063 | 1078.2 | 545.6 | |
| 4.86 | -13.00 | 2.53 | -13.00 | 7.97 | 40.91 | -16.05 | 62.77 | 0.3092 | 918.5 | 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. | |