SDO HMI 2014-11-12 02:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.07 | 64.43 | 11.34 | 36.46 | -8.87 | 323.30 | -26.37 | 114.88 | 0.4859 | 925.0 | 536.6 | |
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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 | 0.69 | 0.00 | 0.39 | -10.59 | 324.64 | -25.03 | 119.30 | 0.4788 | 642.0 | 588.6 | |
| 0.00 | 1.38 | 0.00 | 0.79 | -11.23 | 323.44 | -26.23 | 119.34 | 0.4993 | 808.0 | 629.5 | |
| 8.01 | 52.54 | 4.52 | 29.68 | -8.75 | 323.59 | -26.08 | 114.91 | 0.4810 | 1233.5 | 521.2 | |
| 0.00 | 1.46 | 0.00 | 0.84 | -11.41 | 323.29 | -26.38 | 119.54 | 0.5027 | 631.0 | 488.3 | |
| 7.75 | -3.00 | 4.38 | -3.00 | -8.70 | 323.36 | -26.31 | 114.61 | 0.4839 | 1055.1 | 999999 | |
| 4.31 | -3.00 | 2.44 | -3.00 | -8.64 | 323.13 | -26.54 | 114.32 | 0.4868 | 891.0 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -8.41 | 322.98 | -26.69 | 113.75 | 0.4874 | 601.0 | 584.9 | |
| 0.00 | 2.33 | 0.00 | 1.33 | -9.66 | 322.71 | -26.96 | 115.87 | 0.4988 | 691.0 | 643.6 | |
| 0.00 | 2.15 | 0.00 | 1.22 | -8.50 | 322.80 | -26.86 | 113.80 | 0.4904 | 604.0 | 526.7 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -9.65 | 321.89 | -27.77 | 115.21 | 0.5098 | 666.0 | 425.9 | |
| 0.00 | 1.29 | 0.00 | 0.74 | -7.83 | 321.74 | -27.93 | 111.75 | 0.5016 | 875.0 | 725.1 | |
| 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. | |