SDO HMI 2014-06-06 05:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.93 | 0.00 | 11.29 | 3.84 | 262.10 | -26.79 | 80.00 | 0.4498 | -86.9 | -115.4 | |
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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 | 2.17 | 0.00 | 1.12 | 4.32 | 273.49 | -15.40 | 73.95 | 0.2768 | -1007.0 | -790.4 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 6.27 | 273.25 | -15.64 | 67.65 | 0.2910 | -910.0 | -767.2 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 4.01 | 273.17 | -15.71 | 75.30 | 0.2805 | -778.0 | -582.2 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 3.19 | 272.84 | -16.05 | 78.42 | 0.2830 | -977.0 | -749.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 2.98 | 270.29 | -18.60 | 80.57 | 0.3242 | -840.0 | -668.9 | |
| 0.00 | 3.98 | 0.00 | 2.09 | 2.43 | 270.07 | -18.81 | 82.34 | 0.3265 | -774.0 | -527.9 | |
| 0.00 | 1.81 | 0.00 | 1.05 | 5.29 | 257.74 | -31.15 | 79.77 | 0.5255 | 543.0 | 415.5 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 7.38 | 254.26 | -34.62 | 77.09 | 0.5802 | 696.0 | 559.2 | |
| 0.00 | 1.18 | 0.00 | 0.72 | 2.22 | 253.06 | -35.82 | 86.14 | 0.5883 | 606.0 | 516.8 | |
| 0.00 | 1.00 | 0.00 | 0.63 | 5.06 | 250.75 | -38.14 | 81.78 | 0.6238 | 724.0 | 548.6 | |
| 0.00 | 1.18 | 0.00 | 0.75 | 5.24 | 250.42 | -38.46 | 81.54 | 0.6284 | 588.0 | 507.8 | |
| 0.00 | 1.18 | 0.00 | 0.82 | 0.62 | 244.12 | -44.77 | 89.07 | 0.7066 | 485.0 | 342.0 | |
| 0.00 | 0.72 | 0.00 | 0.51 | 1.44 | 243.93 | -44.95 | 87.91 | 0.7091 | 514.0 | 469.0 | |
| 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. | |