SDO HMI 2014-11-22 13:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.29 | 0.00 | 11.77 | -12.93 | 225.71 | 13.88 | 222.08 | 0.3492 | 507.4 | 133.3 | |
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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 | 1.11 | 0.00 | 0.59 | -11.85 | 228.26 | 16.42 | 229.36 | 0.3662 | 863.0 | 573.8 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -13.42 | 228.33 | 16.49 | 226.30 | 0.3836 | 599.0 | 404.9 | |
| 0.00 | 1.71 | 0.00 | 0.92 | -13.53 | 227.83 | 15.99 | 225.21 | 0.3791 | 953.0 | 828.3 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -12.37 | 227.72 | 15.89 | 227.35 | 0.3651 | 869.0 | 711.3 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -13.65 | 227.61 | 15.78 | 224.60 | 0.3780 | 877.0 | 755.0 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -12.18 | 227.39 | 15.56 | 227.16 | 0.3592 | 875.0 | 616.3 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -13.34 | 227.43 | 15.60 | 224.88 | 0.3725 | 829.0 | 650.1 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -13.37 | 227.15 | 15.32 | 224.31 | 0.3696 | 759.0 | 530.1 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -13.16 | 226.98 | 15.15 | 224.41 | 0.3651 | 938.0 | 811.3 | |
| 0.00 | 1.29 | 0.00 | 0.68 | -12.60 | 226.88 | 15.05 | 225.34 | 0.3578 | 995.0 | 766.7 | |
| 0.00 | 1.37 | 0.00 | 0.73 | -12.94 | 226.75 | 14.91 | 224.41 | 0.3600 | 875.0 | 730.0 | |
| 0.00 | 1.37 | 0.00 | 0.72 | -13.92 | 223.39 | 11.56 | 215.46 | 0.3367 | -953.0 | -761.9 | |
| 0.00 | 5.06 | 0.00 | 2.63 | -12.11 | 222.81 | 10.98 | 217.52 | 0.3072 | -586.0 | -801.3 | |
| 0.00 | 2.23 | 0.00 | 1.17 | -13.79 | 222.83 | 10.99 | 214.35 | 0.3296 | -790.0 | -663.1 | |
| 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. | |