SDO HMI 2014-09-05 04:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.29 | 0.00 | 10.00 | 10.10 | 179.62 | 13.86 | 247.56 | 0.2652 | 4.3 | -30.5 | |
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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 | 2.14 | 0.00 | 1.15 | 12.16 | 188.15 | 22.39 | 284.31 | 0.3860 | -634.0 | -551.4 | |
| 0.00 | 2.77 | 0.00 | 1.48 | 11.51 | 187.83 | 22.07 | 282.76 | 0.3791 | -628.0 | -491.1 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 11.60 | 187.07 | 21.31 | 283.34 | 0.3675 | -684.0 | -569.6 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 11.74 | 186.79 | 21.02 | 283.84 | 0.3633 | -818.0 | -638.8 | |
| 0.00 | 1.16 | 0.00 | 0.62 | 11.17 | 186.67 | 20.91 | 282.33 | 0.3600 | -848.0 | -572.0 | |
| 0.00 | 1.43 | 0.00 | 0.76 | 10.73 | 186.21 | 20.45 | 281.30 | 0.3516 | -736.0 | -534.4 | |
| 0.00 | 0.98 | 0.00 | 0.52 | 11.86 | 186.20 | 20.44 | 284.46 | 0.3545 | -783.0 | -654.0 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 13.47 | 173.46 | 7.69 | 310.06 | 0.1709 | 798.0 | 608.4 | |
| 0.00 | 1.70 | 0.00 | 0.85 | 9.49 | 172.26 | 6.50 | 289.66 | 0.1191 | 925.0 | 674.2 | |
| 0.00 | 2.59 | 0.00 | 1.29 | 2.87 | 169.32 | 3.55 | 219.14 | 0.0986 | 1098.0 | 847.1 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 2.54 | 169.07 | 3.31 | 215.17 | 0.1006 | 895.0 | 814.8 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 12.48 | 163.84 | -1.93 | 19.78 | 0.0974 | 853.0 | 588.6 | |
| 0.00 | 0.63 | 0.00 | 0.31 | 16.48 | 161.09 | -4.67 | 25.89 | 0.1797 | 618.0 | 546.6 | |
| 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. | |