SDO HMI 2014-07-07 21:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.50 | 92.70 | 25.15 | 110.12 | 8.89 | 164.29 | -65.45 | 81.85 | 0.9093 | -411.2 | -47.7 | |
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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 | 1.36 | 0.00 | 1.41 | 9.04 | 168.18 | -61.56 | 81.65 | 0.8796 | -513.0 | -476.4 | |
| 0.00 | 1.18 | 0.00 | 1.22 | 8.74 | 168.20 | -61.54 | 82.00 | 0.8794 | -372.0 | -308.7 | |
| 0.54 | 1.36 | 0.57 | 1.42 | 9.21 | 167.86 | -61.87 | 81.46 | 0.8822 | -339.0 | -273.9 | |
| 0.36 | 2.00 | 0.38 | 2.11 | 8.36 | 167.45 | -62.29 | 82.43 | 0.8855 | 479.2 | 424.8 | |
| 0.54 | 1.72 | 0.61 | 1.93 | 11.49 | 165.89 | -63.85 | 78.95 | 0.8981 | -352.7 | -322.9 | |
| 6.08 | 11.08 | 6.88 | 12.51 | 8.81 | 165.52 | -64.22 | 81.94 | 0.9005 | -684.9 | -481.6 | |
| 1.27 | 3.09 | 1.52 | 3.70 | 10.79 | 163.89 | -65.85 | 79.77 | 0.9125 | 470.2 | 444.5 | |
| 0.00 | 2.18 | 0.00 | 2.55 | 8.91 | 164.61 | -65.13 | 81.83 | 0.9073 | -708.0 | -562.0 | |
| 11.17 | 66.82 | 13.34 | 80.35 | 8.88 | 164.02 | -65.72 | 81.87 | 0.9115 | -540.7 | -9.7 | |
| 1.54 | -9.00 | 1.85 | -9.00 | 8.56 | 163.90 | -65.84 | 82.22 | 0.9124 | -522.8 | 999999 | |
| 0.00 | 0.64 | 0.00 | 0.80 | 10.44 | 162.63 | -67.11 | 80.17 | 0.9212 | 494.0 | 462.4 | |
| 0.00 | 1.27 | 0.00 | 2.12 | 5.14 | 156.75 | -72.99 | 85.73 | 0.9563 | 214.0 | 170.3 | |
| 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. | |