SDO HMI 2013-08-22 19:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.76 | 299.09 | 27.04 | 162.46 | -7.03 | 139.26 | 19.79 | 235.09 | 0.4118 | 843.9 | 362.0 | |
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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 |
| 49.13 | 273.11 | 26.70 | 148.39 | -6.86 | 139.47 | 20.00 | 235.70 | 0.4128 | 1399.5 | 431.8 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -4.92 | 139.30 | 19.83 | 239.53 | 0.3938 | -580.0 | -396.6 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -15.34 | 139.57 | 20.11 | 221.67 | 0.5006 | -682.0 | -513.3 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -9.15 | 138.73 | 19.26 | 230.26 | 0.4254 | 852.0 | 715.8 | |
| 0.00 | 3.86 | 0.00 | 2.20 | -15.78 | 138.32 | 18.85 | 219.26 | 0.4932 | -816.0 | -641.1 | |
| 0.00 | 1.53 | 0.00 | 0.82 | -6.71 | 137.46 | 17.99 | 233.07 | 0.3853 | 998.0 | 798.9 | |
| 0.00 | 2.25 | 0.00 | 1.21 | -7.54 | 137.17 | 17.70 | 230.92 | 0.3900 | 964.0 | 795.4 | |
| 0.63 | 1.71 | 0.34 | 0.92 | -7.76 | 137.08 | 17.61 | 230.35 | 0.3911 | 923.7 | 673.1 | |
| 0.00 | 2.42 | 0.00 | 1.30 | -7.40 | 136.65 | 17.18 | 230.36 | 0.3820 | -191.0 | -89.9 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -7.08 | 136.58 | 17.11 | 230.88 | 0.3779 | -614.0 | -565.9 | |
| 0.00 | 4.04 | 0.00 | 2.16 | -7.39 | 136.43 | 16.96 | 230.00 | 0.3792 | -638.0 | -678.5 | |
| 0.00 | 1.89 | 0.00 | 1.01 | -6.95 | 136.41 | 16.94 | 230.88 | 0.3745 | -961.0 | -761.1 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -4.89 | 135.14 | 15.67 | 233.27 | 0.3373 | -851.0 | -665.2 | |
| 0.00 | 1.35 | 0.00 | 0.73 | -10.21 | 135.24 | 15.77 | 222.61 | 0.3968 | -694.0 | -599.2 | |
| 0.00 | 1.71 | 0.00 | 0.90 | -5.09 | 134.90 | 15.43 | 232.33 | 0.3362 | -759.0 | -599.1 | |
| 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. | |