SDO HMI 2014-12-02 12:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.43 | 0.00 | 9.11 | -5.40 | 96.88 | 16.29 | 246.24 | 0.3047 | 102.0 | 183.7 | |
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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 | 1.20 | 0.00 | 0.66 | -9.59 | 105.52 | 24.94 | 246.86 | 0.4540 | 882.0 | 794.2 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -9.52 | 103.91 | 23.32 | 245.66 | 0.4304 | -831.0 | -550.6 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -3.28 | 102.05 | 21.46 | 259.34 | 0.3733 | 734.0 | 571.3 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -3.10 | 101.82 | 21.23 | 259.71 | 0.3692 | 514.0 | 592.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -3.34 | 101.70 | 21.11 | 259.01 | 0.3679 | 838.0 | 709.7 | |
| 0.00 | 3.93 | 0.00 | 2.09 | -3.27 | 101.47 | 20.89 | 259.07 | 0.3641 | 1060.0 | 864.6 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -3.77 | 100.38 | 19.79 | 257.08 | 0.3482 | 509.0 | 572.2 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -9.43 | 92.87 | 12.28 | 230.04 | 0.2750 | 850.0 | 655.3 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -3.61 | 90.59 | 10.00 | 246.54 | 0.1898 | -859.0 | -649.7 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -4.20 | 90.32 | 9.74 | 243.11 | 0.1900 | -755.0 | -582.0 | |
| 0.00 | 0.94 | 0.00 | 0.47 | -6.07 | 88.52 | 7.93 | 229.31 | 0.1818 | -782.0 | -617.4 | |
| 0.00 | 2.56 | 0.00 | 1.29 | -6.63 | 88.31 | 7.73 | 226.27 | 0.1857 | -936.0 | -691.7 | |
| 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. | |