SDO HMI 2014-08-12 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.07 | 47.26 | 9.72 | 32.46 | -17.84 | 161.42 | 36.89 | 235.64 | 0.6948 | 485.7 | 342.4 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.42 | 26.89 | 3.06 | 18.57 | -16.74 | 162.60 | 38.07 | 237.84 | 0.6998 | 798.9 | 335.7 | |
| 8.39 | -1.00 | 5.79 | -1.00 | -16.85 | 162.43 | 37.89 | 237.58 | 0.6987 | 849.5 | 999999 | |
| 0.81 | 2.35 | 0.56 | 1.61 | -16.85 | 161.95 | 37.41 | 237.26 | 0.6936 | 799.2 | 699.5 | |
| 0.00 | 1.08 | 0.00 | 0.75 | -18.29 | 161.73 | 37.20 | 235.31 | 0.7004 | 592.0 | 471.5 | |
| 0.45 | 5.59 | 0.31 | 3.87 | -19.99 | 160.72 | 36.19 | 232.53 | 0.7014 | 524.6 | 579.4 | |
| 0.00 | 1.08 | 0.00 | 0.74 | -19.46 | 160.31 | 35.77 | 232.86 | 0.6937 | 712.0 | 606.7 | |
| 0.00 | 1.44 | 0.00 | 0.97 | -17.85 | 159.72 | 35.19 | 234.42 | 0.6767 | 462.0 | 425.6 | |
| 0.00 | 0.99 | 0.00 | 0.68 | -19.51 | 160.08 | 35.54 | 232.63 | 0.6917 | 695.0 | 577.3 | |
| 0.00 | 2.35 | 0.00 | 1.59 | -19.06 | 159.46 | 34.92 | 232.71 | 0.6824 | 684.0 | 565.8 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -20.08 | 159.63 | 35.10 | 231.60 | 0.6913 | 727.0 | 689.9 | |
| 0.00 | 0.54 | 0.00 | 0.36 | -20.01 | 158.55 | 34.01 | 230.85 | 0.6801 | -522.0 | -413.3 | |
| 0.00 | 1.89 | 0.00 | 1.26 | -19.24 | 158.13 | 33.60 | 231.46 | 0.6703 | -633.0 | -443.7 | |
| 0.00 | 0.99 | 0.00 | 0.66 | -20.38 | 157.51 | 32.98 | 229.56 | 0.6726 | -539.0 | -467.3 | |
| 0.00 | 0.90 | 0.00 | 0.60 | -20.49 | 157.23 | 32.69 | 229.19 | 0.6708 | -613.0 | -516.9 | |
| 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. | |