SDO HMI 2014-10-10 20:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.14 | 19.08 | 0.60 | 10.06 | -13.22 | 58.44 | 3.45 | 190.32 | 0.3468 | -86.4 | -26.8 | |
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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 | 1.05 | 0.00 | 0.56 | -14.42 | 64.03 | 9.04 | 203.45 | 0.3840 | 678.0 | 540.7 | |
| 0.00 | 1.40 | 0.00 | 0.74 | -13.29 | 62.93 | 7.94 | 202.01 | 0.3601 | 906.0 | 777.1 | |
| 0.00 | 2.63 | 0.00 | 1.38 | -12.59 | 60.93 | 5.94 | 197.44 | 0.3384 | 922.0 | 767.2 | |
| 0.00 | 3.41 | 0.00 | 1.79 | -12.43 | 60.49 | 5.50 | 196.37 | 0.3337 | 781.0 | 471.4 | |
| 0.00 | 0.79 | 0.00 | 0.41 | -12.02 | 60.36 | 5.37 | 196.36 | 0.3266 | -845.0 | -719.0 | |
| 1.14 | 3.94 | 0.60 | 2.06 | -12.10 | 59.11 | 4.12 | 192.62 | 0.3227 | -1019.0 | -803.4 | |
| 0.00 | 0.96 | 0.00 | 0.51 | -13.11 | 58.63 | 3.64 | 190.60 | 0.3374 | -850.0 | -706.3 | |
| 0.00 | 1.49 | 0.00 | 0.78 | -13.27 | 58.60 | 3.61 | 190.43 | 0.3399 | -859.0 | -719.1 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -17.99 | 53.80 | -1.19 | 177.24 | 0.4118 | 711.0 | 490.5 | |
| 0.00 | 1.66 | 0.00 | 0.89 | -15.14 | 48.38 | -6.61 | 162.98 | 0.3812 | -853.0 | -719.5 | |
| 0.00 | 0.70 | 0.00 | 0.37 | -13.08 | 46.77 | -8.22 | 157.06 | 0.3588 | -895.0 | -769.9 | |
| 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. | |