SDO HMI 2011-12-16 08:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.98 | 58.47 | 7.69 | 30.14 | -17.00 | 323.76 | 0.13 | 180.56 | 0.2774 | -204.1 | -57.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.70 | 0.00 | 0.87 | -14.72 | 327.13 | 3.49 | 193.99 | 0.2450 | 878.0 | 712.3 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -14.48 | 326.94 | 3.31 | 193.51 | 0.2403 | 870.0 | 675.6 | |
| 0.00 | 4.77 | 0.00 | 2.46 | -17.29 | 326.40 | 2.77 | 189.35 | 0.2850 | 1152.0 | 933.1 | |
| 1.62 | 3.83 | 0.83 | 1.98 | -17.41 | 324.85 | 1.22 | 184.13 | 0.2840 | 996.9 | 857.8 | |
| 0.00 | 6.47 | 0.00 | 3.35 | -17.97 | 324.73 | 1.10 | 183.59 | 0.2932 | 1062.0 | 701.5 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -16.58 | 324.23 | 0.60 | 182.15 | 0.2695 | 881.0 | 698.2 | |
| 0.00 | 1.70 | 0.00 | 0.88 | -18.46 | 324.02 | 0.39 | 181.23 | 0.3009 | 930.0 | 795.7 | |
| 11.49 | 14.21 | 5.89 | 7.29 | -15.97 | 323.83 | 0.20 | 180.75 | 0.2590 | -1106.5 | -648.4 | |
| 0.00 | 1.53 | 0.00 | 0.79 | -17.72 | 323.62 | -0.01 | 179.95 | 0.2884 | 927.0 | 656.2 | |
| 0.00 | 2.38 | 0.00 | 1.22 | -16.46 | 323.19 | -0.45 | 178.40 | 0.2674 | -1057.0 | -894.3 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -17.51 | 322.81 | -0.82 | 177.25 | 0.2852 | -881.0 | -651.3 | |
| 0.00 | 2.89 | 0.00 | 1.49 | -16.92 | 322.63 | -1.00 | 176.51 | 0.2755 | -853.0 | -866.7 | |
| 0.00 | 6.21 | 0.00 | 3.20 | -17.11 | 322.44 | -1.19 | 175.91 | 0.2788 | -1003.0 | -735.7 | |
| 1.87 | 9.28 | 0.97 | 4.81 | -17.91 | 321.66 | -1.97 | 173.58 | 0.2934 | -1062.9 | -903.5 | |
| 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. | |