SDO HMI 2014-10-04 08:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.11 | 34.58 | 1.09 | 18.12 | -12.16 | 139.73 | -1.02 | 177.08 | 0.3229 | -37.6 | 251.5 | |
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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 | 2.64 | 0.00 | 1.38 | -11.46 | 142.41 | 1.65 | 185.23 | 0.3119 | 777.0 | 644.4 | |
| 2.11 | 13.64 | 1.09 | 7.05 | -9.98 | 140.39 | -0.36 | 178.75 | 0.2859 | 1180.8 | 822.2 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -16.16 | 140.28 | -0.47 | 178.82 | 0.3879 | 755.0 | 657.4 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -15.97 | 140.22 | -0.53 | 178.66 | 0.3848 | 764.0 | 713.5 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -9.54 | 140.18 | -0.57 | 177.96 | 0.2786 | 1065.0 | 860.5 | |
| 0.00 | 1.58 | 0.00 | 0.82 | -11.39 | 139.96 | -0.79 | 177.47 | 0.3098 | 800.0 | 647.5 | |
| 0.00 | 1.76 | 0.00 | 0.94 | -15.25 | 139.10 | -1.65 | 175.72 | 0.3741 | -820.0 | -706.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -14.80 | 138.92 | -1.83 | 175.14 | 0.3670 | -997.0 | -827.4 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -15.00 | 138.92 | -1.84 | 175.19 | 0.3702 | -777.0 | -729.6 | |
| 0.00 | 2.38 | 0.00 | 1.27 | -15.51 | 138.41 | -2.34 | 174.02 | 0.3793 | -818.0 | -629.9 | |
| 0.00 | 2.11 | 0.00 | 1.08 | -8.42 | 138.48 | -2.27 | 171.38 | 0.2625 | 575.0 | 592.7 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -15.26 | 138.32 | -2.43 | 173.72 | 0.3753 | -870.0 | -740.0 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -14.84 | 137.89 | -2.86 | 172.47 | 0.3694 | -778.0 | -649.4 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -15.16 | 137.80 | -2.96 | 172.33 | 0.3748 | -725.0 | -449.2 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -14.68 | 137.65 | -3.10 | 171.77 | 0.3674 | -805.0 | -739.9 | |
| 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. | |