SDO HMI 2011-11-11 18:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.32 | 344.40 | 29.53 | 194.58 | 28.06 | 44.18 | -15.23 | 28.86 | 0.4827 | -1060.5 | -416.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.20 | 0.00 | 0.69 | 31.34 | 46.71 | -12.70 | 21.72 | 0.5096 | -903.0 | -790.4 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 31.17 | 46.63 | -12.79 | 21.99 | 0.5078 | -823.0 | -700.6 | |
| 0.00 | 1.98 | 0.00 | 1.14 | 31.47 | 46.34 | -13.08 | 22.18 | 0.5135 | -719.0 | -546.0 | |
| 0.00 | 1.55 | 0.00 | 0.94 | 35.57 | 43.80 | -15.62 | 22.23 | 0.5811 | -696.0 | -501.8 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 33.38 | 43.96 | -15.46 | 23.86 | 0.5524 | -677.0 | -533.7 | |
| 44.32 | 328.66 | 24.98 | 185.39 | 27.85 | 44.28 | -15.13 | 28.93 | 0.4791 | -1340.3 | -413.7 | |
| 1.46 | -6.00 | 0.83 | -6.00 | 28.38 | 44.17 | -15.24 | 28.51 | 0.4867 | -660.2 | 999999 | |
| 2.07 | -6.00 | 1.17 | -6.00 | 28.54 | 44.01 | -15.41 | 28.58 | 0.4900 | -478.7 | 999999 | |
| 3.01 | -6.00 | 1.71 | -6.00 | 28.27 | 43.87 | -15.54 | 29.08 | 0.4876 | -841.0 | 999999 | |
| 0.00 | 1.29 | 0.00 | 0.80 | 36.56 | 41.59 | -17.83 | 24.06 | 0.6056 | -831.0 | -679.5 | |
| 1.46 | 2.24 | 0.84 | 1.28 | 28.37 | 41.82 | -17.60 | 31.96 | 0.5047 | -811.2 | -740.0 | |
| 0.00 | 3.27 | 0.00 | 1.89 | 29.03 | 41.45 | -17.96 | 31.69 | 0.5154 | -783.0 | -645.6 | |
| 0.00 | 0.69 | 0.00 | 0.40 | 27.63 | 38.39 | -21.02 | 37.41 | 0.5253 | 608.0 | 543.1 | |
| 0.00 | 1.29 | 0.00 | 0.75 | 26.97 | 38.13 | -21.29 | 38.60 | 0.5206 | 673.0 | 536.9 | |
| 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. | |