SDO HMI 2011-10-14 01:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.77 | 101.53 | 15.61 | 55.05 | 19.90 | 98.11 | 20.11 | 307.41 | 0.4087 | -202.2 | -211.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.71 | 11.81 | 1.48 | 6.45 | 20.17 | 99.23 | 21.24 | 306.52 | 0.4250 | -771.3 | -554.0 | |
| 16.88 | 57.01 | 9.18 | 31.02 | 19.57 | 98.91 | 20.92 | 305.66 | 0.4158 | -1033.2 | -462.9 | |
| 1.22 | 3.06 | 0.67 | 1.67 | 20.07 | 98.67 | 20.68 | 306.97 | 0.4170 | -789.3 | -689.7 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 19.80 | 98.33 | 20.34 | 306.84 | 0.4104 | -857.0 | -706.2 | |
| 0.00 | 0.87 | 0.00 | 0.47 | 19.42 | 97.91 | 19.92 | 306.56 | 0.4017 | -867.0 | -661.7 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 18.78 | 97.53 | 19.54 | 305.67 | 0.3914 | 795.0 | 628.8 | |
| 0.00 | 1.22 | 0.00 | 0.66 | 19.07 | 97.13 | 19.13 | 306.82 | 0.3887 | -916.0 | -674.0 | |
| 0.00 | 1.66 | 0.00 | 0.89 | 19.42 | 96.93 | 18.94 | 307.83 | 0.3893 | -666.0 | -415.7 | |
| 7.17 | 13.64 | 3.86 | 7.34 | 21.03 | 95.96 | 17.96 | 312.56 | 0.3925 | 1017.0 | 776.6 | |
| 0.79 | 3.59 | 0.42 | 1.92 | 20.44 | 95.85 | 17.86 | 311.52 | 0.3854 | 1036.7 | 810.6 | |
| 0.00 | 1.22 | 0.00 | 0.65 | 20.06 | 95.04 | 17.05 | 311.96 | 0.3719 | 653.0 | 528.6 | |
| 0.00 | 1.49 | 0.00 | 0.79 | 20.25 | 94.93 | 16.93 | 312.54 | 0.3725 | 787.0 | 667.5 | |
| 0.00 | 2.54 | 0.00 | 1.35 | 20.04 | 94.74 | 16.74 | 312.39 | 0.3681 | 968.0 | 905.9 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 20.32 | 94.73 | 16.74 | 312.99 | 0.3709 | 683.0 | 601.8 | |
| 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. | |