SDO HMI 2014-11-10 18:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.14 | 0.00 | 10.11 | -9.84 | 337.27 | -30.00 | 114.14 | 0.5417 | -74.3 | -120.3 | |
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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 | 0.78 | 0.00 | 0.44 | -9.98 | 342.49 | -24.77 | 118.67 | 0.4723 | 839.0 | 694.8 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -5.11 | 342.57 | -24.70 | 108.86 | 0.4417 | 857.0 | 673.4 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -10.05 | 341.05 | -26.22 | 117.47 | 0.4923 | 581.0 | 485.5 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -12.57 | 340.59 | -26.68 | 121.51 | 0.5160 | 755.0 | 558.8 | |
| 0.00 | 1.98 | 0.00 | 1.12 | -6.79 | 340.36 | -26.91 | 110.74 | 0.4825 | 681.0 | 542.0 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -6.90 | 339.85 | -27.42 | 110.58 | 0.4904 | 592.0 | 517.6 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -9.98 | 337.02 | -30.25 | 114.20 | 0.5461 | -238.0 | -305.2 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -10.02 | 336.41 | -30.85 | 113.87 | 0.5544 | -699.0 | -597.6 | |
| 0.00 | 2.33 | 0.00 | 1.40 | -12.09 | 336.10 | -31.17 | 117.03 | 0.5704 | -792.0 | -591.7 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -10.89 | 335.11 | -32.16 | 114.43 | 0.5763 | -699.0 | -655.5 | |
| 0.00 | 1.29 | 0.00 | 0.78 | -9.51 | 335.20 | -32.07 | 112.24 | 0.5680 | -815.0 | -640.8 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -10.13 | 335.13 | -32.14 | 113.21 | 0.5720 | -645.0 | -555.1 | |
| 0.00 | 1.55 | 0.00 | 0.95 | -10.58 | 334.10 | -33.16 | 113.32 | 0.5878 | -465.0 | -409.1 | |
| 0.00 | 0.95 | 0.00 | 0.58 | -10.26 | 333.86 | -33.41 | 112.65 | 0.5894 | -628.0 | -437.2 | |
| 0.00 | 0.86 | 0.00 | 0.53 | -10.64 | 333.48 | -33.79 | 113.02 | 0.5961 | -438.0 | -319.5 | |
| 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. | |