SDO HMI 2014-08-12 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.96 | 46.48 | 12.01 | 32.92 | -17.93 | 161.34 | 39.00 | 236.92 | 0.7170 | 550.4 | 359.8 | |
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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 |
| 0.00 | 1.08 | 0.00 | 0.83 | -17.96 | 165.94 | 43.60 | 239.64 | 0.7626 | 460.0 | 432.3 | |
| 11.37 | 22.39 | 8.12 | 15.96 | -16.73 | 162.55 | 40.21 | 239.19 | 0.7222 | 838.9 | 458.0 | |
| 0.00 | 2.26 | 0.00 | 1.63 | -18.17 | 162.47 | 40.13 | 237.37 | 0.7295 | 331.0 | 289.6 | |
| 0.36 | 1.26 | 0.26 | 0.89 | -16.78 | 161.94 | 39.60 | 238.75 | 0.7161 | 657.5 | 600.2 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -18.00 | 161.02 | 38.68 | 236.66 | 0.7137 | 534.0 | 576.3 | |
| 0.00 | 2.08 | 0.00 | 1.48 | -19.04 | 161.22 | 38.88 | 235.52 | 0.7220 | 61.0 | 135.4 | |
| 0.00 | 1.53 | 0.00 | 1.09 | -19.74 | 160.62 | 38.28 | 234.30 | 0.7204 | 716.0 | 596.6 | |
| 0.00 | 0.90 | 0.00 | 0.64 | -19.97 | 160.65 | 38.31 | 234.03 | 0.7222 | 449.0 | 415.8 | |
| 4.15 | 8.67 | 2.89 | 6.04 | -19.08 | 159.51 | 37.17 | 234.32 | 0.7052 | 854.8 | 666.2 | |
| 0.00 | 1.26 | 0.00 | 0.89 | -19.97 | 159.75 | 37.41 | 233.41 | 0.7134 | 826.0 | 623.6 | |
| 1.08 | 2.71 | 0.74 | 1.86 | -19.26 | 158.19 | 35.85 | 233.16 | 0.6931 | -677.5 | -534.9 | |
| 0.00 | 1.17 | 0.00 | 0.80 | -20.35 | 157.47 | 35.13 | 231.30 | 0.6936 | -382.0 | -342.3 | |
| 0.00 | 0.90 | 0.00 | 0.62 | -20.40 | 157.25 | 34.91 | 231.07 | 0.6918 | -491.0 | -466.8 | |
| 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. | |