SDO HMI 2014-12-07 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 24.04 | 0.00 | 12.40 | 14.51 | 15.22 | -0.56 | 358.72 | 0.2641 | -438.5 | -428.1 | |
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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 | 1.19 | 0.00 | 0.62 | 15.69 | 25.56 | 9.78 | 328.72 | 0.3162 | -804.0 | -656.1 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 17.79 | 23.61 | 7.82 | 336.93 | 0.3320 | -728.0 | -559.2 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 12.62 | 21.28 | 5.49 | 336.74 | 0.2373 | -949.0 | -795.2 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 10.06 | 17.89 | 2.10 | 348.25 | 0.1778 | -913.0 | -684.4 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 12.59 | 17.45 | 1.67 | 352.54 | 0.2195 | -809.0 | -619.7 | |
| 0.00 | 1.88 | 0.00 | 0.95 | 12.17 | 17.33 | 1.54 | 352.84 | 0.2120 | -1033.0 | -855.1 | |
| 0.00 | 4.01 | 0.00 | 2.02 | 10.00 | 17.26 | 1.47 | 351.67 | 0.1749 | -755.0 | -720.8 | |
| 0.00 | 3.75 | 0.00 | 1.91 | 13.17 | 17.13 | 1.34 | 354.27 | 0.2286 | -774.0 | -669.8 | |
| 0.00 | 2.05 | 0.00 | 1.05 | 15.70 | 13.06 | -2.72 | 9.65 | 0.2744 | -711.0 | -620.3 | |
| 0.00 | 2.13 | 0.00 | 1.11 | 17.71 | 12.17 | -3.62 | 11.24 | 0.3101 | -563.0 | -347.4 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.53 | 10.03 | -5.76 | 17.71 | 0.3161 | 846.0 | 635.3 | |
| 0.00 | 2.05 | 0.00 | 1.10 | 19.71 | 4.37 | -11.42 | 29.02 | 0.3859 | 759.0 | 695.8 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 24.44 | 359.05 | -16.73 | 32.44 | 0.4907 | 734.0 | 597.4 | |
| 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. | |