SDO HMI 2014-11-14 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 12.63 | 0.00 | 6.85 | -9.37 | 337.13 | 20.39 | 238.23 | 0.4052 | -525.9 | -363.2 | |
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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 | 1.20 | 0.00 | 0.68 | -7.03 | 342.96 | 26.22 | 249.09 | 0.4714 | 718.0 | 632.1 | |
| 0.00 | 1.29 | 0.00 | 0.73 | -10.91 | 341.85 | 25.11 | 240.65 | 0.4800 | 641.0 | 553.1 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -9.30 | 339.19 | 22.45 | 241.12 | 0.4322 | -664.0 | -477.4 | |
| 0.00 | 1.20 | 0.00 | 0.65 | -9.75 | 337.63 | 20.89 | 238.42 | 0.4143 | -746.0 | -541.6 | |
| 0.00 | 1.38 | 0.00 | 0.75 | -10.02 | 337.45 | 20.72 | 237.64 | 0.4141 | -770.0 | -578.6 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -9.63 | 335.83 | 19.09 | 236.37 | 0.3889 | -848.0 | -691.3 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -7.86 | 335.29 | 18.55 | 239.67 | 0.3668 | -798.0 | -606.8 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -9.25 | 335.27 | 18.53 | 236.42 | 0.3781 | -692.0 | -552.9 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -8.94 | 334.84 | 18.10 | 236.51 | 0.3696 | -807.0 | -556.5 | |
| 0.00 | 1.20 | 0.00 | 0.64 | -10.74 | 333.67 | 16.94 | 230.72 | 0.3713 | -795.0 | -612.6 | |
| 0.00 | 1.38 | 0.00 | 0.73 | -8.95 | 333.49 | 16.75 | 234.43 | 0.3515 | -1024.0 | -812.8 | |
| 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. | |