SDO HMI 2014-05-19 16:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.75 | 239.64 | 23.86 | 147.38 | -24.55 | 190.63 | 29.62 | 229.37 | 0.5945 | 676.1 | 311.3 | |
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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 |
| 37.40 | 225.87 | 23.04 | 139.10 | -24.48 | 190.88 | 29.87 | 229.71 | 0.5964 | 1190.4 | 356.7 | |
| 0.00 | 0.54 | 0.00 | 0.34 | -26.19 | 191.04 | 30.03 | 227.47 | 0.6115 | 581.0 | 454.3 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -23.05 | 189.84 | 28.83 | 230.87 | 0.5741 | 461.0 | 487.2 | |
| 1.35 | -1.00 | 0.82 | -1.00 | -24.16 | 190.00 | 28.98 | 229.40 | 0.5845 | 786.0 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.90 | -26.57 | 190.56 | 29.55 | 226.56 | 0.6096 | 521.0 | 462.6 | |
| 0.00 | 0.90 | 0.00 | 0.52 | -19.79 | 188.24 | 27.23 | 234.52 | 0.5307 | -679.0 | -569.6 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -26.78 | 189.65 | 28.63 | 225.47 | 0.6023 | 591.0 | 504.5 | |
| 0.00 | 0.45 | 0.00 | 0.27 | -26.04 | 186.19 | 25.17 | 223.13 | 0.5612 | -553.0 | -478.4 | |
| 0.00 | 2.61 | 0.00 | 1.56 | -26.31 | 185.91 | 24.90 | 222.48 | 0.5610 | -809.0 | -689.0 | |
| 0.00 | 1.98 | 0.00 | 1.18 | -26.01 | 185.81 | 24.80 | 222.77 | 0.5572 | -1026.0 | -773.6 | |
| 0.00 | 1.62 | 0.00 | 0.97 | -27.15 | 185.32 | 24.31 | 220.73 | 0.5635 | -871.0 | -709.7 | |
| 0.00 | 0.90 | 0.00 | 0.54 | -27.35 | 185.26 | 24.24 | 220.40 | 0.5649 | -641.0 | -588.5 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -27.45 | 185.13 | 24.12 | 220.13 | 0.5648 | -696.0 | -636.7 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -28.43 | 179.79 | 18.78 | 212.51 | 0.5289 | -706.0 | -548.8 | |
| 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. | |