SDO HMI 2014-05-16 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.34 | 301.74 | 28.56 | 161.85 | -24.02 | 192.15 | -6.88 | 163.54 | 0.3849 | 793.0 | 363.7 | |
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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 | 1.53 | 0.00 | 0.79 | -19.58 | 195.31 | -3.73 | 168.23 | 0.3015 | -927.0 | -790.4 | |
| 20.38 | 284.66 | 10.90 | 152.42 | -23.74 | 192.76 | -6.27 | 164.59 | 0.3777 | 1427.3 | 423.5 | |
| 4.85 | -2.00 | 2.59 | -2.00 | -23.71 | 192.37 | -6.67 | 163.64 | 0.3790 | 1363.1 | 999999 | |
| 24.07 | -2.00 | 12.91 | -2.00 | -24.07 | 192.31 | -6.72 | 163.81 | 0.3847 | 1123.8 | 999999 | |
| 2.78 | -2.00 | 1.49 | -2.00 | -23.90 | 191.89 | -7.14 | 162.71 | 0.3842 | 862.2 | 999999 | |
| 1.26 | -2.00 | 0.67 | -2.00 | -23.90 | 191.49 | -7.54 | 161.81 | 0.3861 | 712.1 | 999999 | |
| 0.00 | 3.59 | 0.00 | 1.93 | -23.54 | 190.94 | -8.09 | 160.25 | 0.3835 | 600.0 | 561.2 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -25.00 | 186.46 | -12.57 | 152.79 | 0.4332 | -620.0 | -451.7 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -29.75 | 185.89 | -13.14 | 156.72 | 0.5015 | -749.0 | -595.6 | |
| 0.00 | 5.21 | 0.00 | 2.92 | -27.28 | 185.71 | -13.32 | 154.02 | 0.4694 | -823.0 | -719.1 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -27.85 | 185.57 | -13.46 | 154.38 | 0.4779 | -839.0 | -688.6 | |
| 0.00 | 1.44 | 0.00 | 0.81 | -27.71 | 185.31 | -13.73 | 153.81 | 0.4779 | -827.0 | -727.8 | |
| 0.00 | 1.35 | 0.00 | 0.75 | -25.38 | 185.32 | -13.72 | 151.22 | 0.4468 | -706.0 | -611.9 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -30.40 | 182.82 | -16.21 | 152.84 | 0.5297 | -681.0 | -547.6 | |
| 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. | |