SDO HMI 2014-09-16 02:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.91 | 0.00 | 10.15 | 7.77 | 342.30 | -39.31 | 86.50 | 0.6301 | -530.0 | -417.8 | |
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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 | 0.89 | 0.00 | 0.54 | 7.73 | 345.21 | -36.40 | 86.74 | 0.5912 | -713.0 | -531.7 | |
| 0.00 | 1.16 | 0.00 | 0.71 | 9.95 | 344.88 | -36.73 | 82.99 | 0.5957 | 492.0 | 363.5 | |
| 0.00 | 1.16 | 0.00 | 0.71 | 7.83 | 344.89 | -36.71 | 86.56 | 0.5955 | -626.0 | -505.8 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 8.24 | 344.24 | -37.37 | 85.86 | 0.6044 | -716.0 | -561.5 | |
| 0.00 | 1.16 | 0.00 | 0.72 | 7.77 | 344.06 | -37.55 | 86.62 | 0.6071 | -747.0 | -563.3 | |
| 0.00 | 1.24 | 0.00 | 0.78 | 7.56 | 343.23 | -38.38 | 86.93 | 0.6186 | -694.0 | -557.6 | |
| 0.00 | 1.24 | 0.00 | 0.79 | 7.37 | 342.82 | -38.79 | 87.20 | 0.6242 | -706.0 | -580.6 | |
| 0.00 | 1.42 | 0.00 | 0.90 | 7.52 | 342.80 | -38.80 | 86.96 | 0.6244 | -721.0 | -478.2 | |
| 0.00 | 0.98 | 0.00 | 0.62 | 6.38 | 342.87 | -38.73 | 88.80 | 0.6242 | -633.0 | -505.5 | |
| 0.00 | 0.71 | 0.00 | 0.45 | 7.24 | 342.68 | -38.93 | 87.40 | 0.6262 | -682.0 | -608.1 | |
| 0.00 | 1.24 | 0.00 | 0.79 | 7.66 | 342.59 | -39.01 | 86.73 | 0.6271 | -701.0 | -556.6 | |
| 0.00 | 0.89 | 0.00 | 0.57 | 7.78 | 342.26 | -39.34 | 86.51 | 0.6315 | -559.0 | -462.6 | |
| 0.00 | 0.89 | 0.00 | 0.57 | 8.13 | 341.99 | -39.62 | 85.96 | 0.6351 | -600.0 | -476.0 | |
| 0.00 | 0.89 | 0.00 | 0.62 | 8.76 | 336.17 | -45.43 | 84.79 | 0.7093 | -621.0 | -535.8 | |
| 0.00 | 0.80 | 0.00 | 0.61 | 6.34 | 331.90 | -49.70 | 87.81 | 0.7609 | 277.0 | 335.8 | |
| 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. | |