SDO HMI 2014-11-14 02:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.25 | 0.00 | 8.60 | -9.78 | 338.98 | 15.68 | 229.75 | 0.3509 | 80.2 | -46.1 | |
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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 | 0.61 | -5.38 | 345.88 | 22.58 | 249.68 | 0.4093 | 877.0 | 723.4 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -7.46 | 343.05 | 19.75 | 241.99 | 0.3811 | 901.0 | 759.3 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -7.73 | 342.97 | 19.67 | 241.26 | 0.3820 | 747.0 | 544.3 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -10.04 | 342.10 | 18.80 | 234.94 | 0.3894 | 792.0 | 692.3 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -10.41 | 341.93 | 18.63 | 233.93 | 0.3905 | 682.0 | 653.4 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -10.76 | 340.97 | 17.67 | 231.75 | 0.3814 | 813.0 | 648.4 | |
| 0.00 | 0.69 | 0.00 | 0.37 | -10.53 | 340.51 | 17.21 | 231.50 | 0.3734 | 170.0 | 281.5 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -9.91 | 337.63 | 14.33 | 227.74 | 0.3309 | -668.0 | -506.3 | |
| 0.00 | 1.63 | 0.00 | 0.86 | -12.58 | 336.14 | 12.84 | 219.08 | 0.3456 | -942.0 | -749.4 | |
| 0.00 | 1.55 | 0.00 | 0.82 | -12.80 | 336.06 | 12.76 | 218.50 | 0.3474 | -737.0 | -577.1 | |
| 0.00 | 3.36 | 0.00 | 1.74 | -8.99 | 334.94 | 11.64 | 223.99 | 0.2883 | -874.0 | -737.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -11.00 | 334.71 | 11.41 | 218.89 | 0.3106 | -798.0 | -619.7 | |
| 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. | |