SDO HMI 2011-11-19 02:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.65 | 0.00 | 11.27 | 17.53 | 313.31 | -9.41 | 29.79 | 0.3097 | -846.4 | -666.8 | |
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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 | 1.12 | 0.00 | 0.57 | 17.51 | 318.38 | -4.34 | 15.49 | 0.2717 | -741.0 | -605.0 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 18.19 | 317.55 | -5.17 | 17.48 | 0.2865 | -667.0 | -536.7 | |
| 0.00 | 2.49 | 0.00 | 1.28 | 17.91 | 317.47 | -5.26 | 18.07 | 0.2825 | -1001.0 | -853.7 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 17.88 | 316.72 | -6.01 | 20.47 | 0.2861 | -962.0 | -791.9 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 17.57 | 316.35 | -6.37 | 22.02 | 0.2835 | -910.0 | -701.1 | |
| 0.00 | 2.15 | 0.00 | 1.09 | 13.07 | 316.15 | -6.57 | 31.06 | 0.2171 | -984.0 | -742.6 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 17.32 | 315.77 | -6.96 | 24.18 | 0.2836 | -736.0 | -546.9 | |
| 0.00 | 1.80 | 0.00 | 0.94 | 19.44 | 314.35 | -8.38 | 25.10 | 0.3252 | -821.0 | -557.5 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 16.19 | 311.37 | -11.35 | 38.36 | 0.3060 | -981.0 | -674.8 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 17.26 | 311.21 | -11.51 | 36.56 | 0.3214 | -656.0 | -577.9 | |
| 0.00 | 2.32 | 0.00 | 1.22 | 18.14 | 309.75 | -12.98 | 38.11 | 0.3473 | -870.0 | -656.4 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 18.13 | 308.53 | -14.19 | 40.59 | 0.3598 | -918.0 | -702.8 | |
| 0.00 | 1.03 | 0.00 | 0.55 | 18.19 | 308.33 | -14.39 | 40.85 | 0.3626 | -783.0 | -606.5 | |
| 0.00 | 1.55 | 0.00 | 0.83 | 19.34 | 305.98 | -16.74 | 42.88 | 0.4012 | -819.0 | -679.2 | |
| 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. | |