SDO HMI 2014-12-07 01:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.74 | 0.00 | 11.28 | 14.56 | 14.89 | -5.82 | 356.22 | 0.2792 | -374.3 | -410.9 | |
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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 | 1.02 | 0.00 | 0.53 | 15.42 | 25.19 | 4.49 | 344.01 | 0.2753 | -830.0 | -683.9 | |
| 0.00 | 2.13 | 0.00 | 1.09 | 13.86 | 22.85 | 2.14 | 351.30 | 0.2411 | -681.0 | -514.0 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 22.29 | 18.21 | -2.50 | 6.10 | 0.3808 | -841.0 | -665.9 | |
| 0.00 | 1.28 | 0.00 | 0.64 | 10.28 | 18.19 | -2.51 | 13.77 | 0.1820 | -1137.0 | -914.0 | |
| 0.00 | 2.05 | 0.00 | 1.03 | 9.92 | 17.77 | -2.93 | 16.52 | 0.1779 | -998.0 | -749.1 | |
| 0.00 | 0.94 | 0.00 | 0.47 | 9.71 | 17.65 | -3.05 | 17.51 | 0.1751 | -897.0 | -730.2 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 12.30 | 17.06 | -3.65 | 16.45 | 0.2205 | -798.0 | -669.0 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 12.05 | 16.70 | -4.01 | 18.32 | 0.2184 | -797.0 | -586.8 | |
| 0.00 | 7.08 | 0.00 | 3.62 | 13.57 | 15.67 | -5.04 | 20.18 | 0.2485 | -545.0 | -614.0 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 19.96 | 4.32 | -16.38 | 38.01 | 0.4323 | 576.0 | 477.7 | |
| 0.00 | 1.02 | 0.00 | 0.56 | 19.75 | 4.31 | -16.39 | 38.36 | 0.4298 | 872.0 | 727.3 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 20.15 | 4.27 | -16.44 | 37.81 | 0.4351 | 477.0 | 494.9 | |
| 0.00 | 1.19 | 0.00 | 0.68 | 20.03 | 358.78 | -21.92 | 45.86 | 0.4907 | 733.0 | 584.1 | |
| 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. | |