SDO HMI 2014-10-11 00:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.75 | 0.00 | 12.81 | 12.25 | 96.07 | 43.28 | 281.84 | 0.6844 | 46.2 | -153.2 | |
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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 | 3.07 | 0.00 | 2.29 | 10.65 | 101.64 | 48.86 | 278.76 | 0.7512 | -634.0 | -442.8 | |
| 0.00 | 2.36 | 0.00 | 1.77 | 10.89 | 101.60 | 48.82 | 279.09 | 0.7508 | -594.0 | -508.7 | |
| 0.00 | 0.70 | 0.00 | 0.52 | 11.21 | 101.35 | 48.57 | 279.53 | 0.7481 | -431.0 | -392.6 | |
| 0.00 | 1.93 | 0.00 | 1.42 | 11.19 | 100.93 | 48.15 | 279.51 | 0.7432 | -546.0 | -488.2 | |
| 0.00 | 2.72 | 0.00 | 1.84 | 10.51 | 96.02 | 43.23 | 278.79 | 0.6838 | -663.0 | -509.5 | |
| 0.00 | 1.05 | 0.00 | 0.71 | 10.51 | 95.52 | 42.73 | 278.83 | 0.6775 | -664.0 | -599.2 | |
| 0.00 | 1.05 | 0.00 | 0.69 | 11.41 | 93.91 | 41.12 | 280.31 | 0.6576 | 578.0 | 554.0 | |
| 0.00 | 0.96 | 0.00 | 0.59 | 15.76 | 88.44 | 35.66 | 288.32 | 0.5932 | 608.0 | 467.5 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 14.38 | 87.60 | 34.82 | 286.25 | 0.5783 | 396.0 | 421.8 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 15.10 | 87.66 | 34.88 | 287.47 | 0.5810 | 657.0 | 529.8 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 15.75 | 87.48 | 34.70 | 288.63 | 0.5804 | 560.0 | 487.7 | |
| 0.00 | 1.49 | 0.00 | 0.90 | 15.53 | 87.06 | 34.28 | 288.40 | 0.5741 | 803.0 | 685.8 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 18.63 | 87.61 | 34.83 | 293.37 | 0.5918 | 531.0 | 380.3 | |
| 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. | |