SDO HMI 2014-09-06 20:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.63 | 87.69 | 18.10 | 47.09 | -14.71 | 149.22 | 5.47 | 193.97 | 0.3863 | -133.8 | 48.0 | |
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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 |
| 0.00 | 3.48 | 0.00 | 1.90 | -16.57 | 149.90 | 6.15 | 194.28 | 0.4177 | -710.0 | -595.2 | |
| 11.33 | 49.60 | 6.02 | 26.38 | -13.17 | 149.49 | 5.74 | 195.62 | 0.3632 | 1189.7 | 514.2 | |
| 4.01 | 29.35 | 2.18 | 15.97 | -16.56 | 149.39 | 5.64 | 193.15 | 0.4157 | -1038.3 | -757.3 | |
| 2.23 | -2.00 | 1.19 | -2.00 | -13.49 | 149.25 | 5.50 | 194.76 | 0.3672 | 1033.3 | 999999 | |
| 2.23 | -2.00 | 1.19 | -2.00 | -13.65 | 149.22 | 5.47 | 194.58 | 0.3696 | 750.1 | 999999 | |
| 1.43 | -3.00 | 0.78 | -3.00 | -16.86 | 149.30 | 5.55 | 192.79 | 0.4200 | -768.6 | 999999 | |
| 1.16 | -2.00 | 0.62 | -2.00 | -13.42 | 149.06 | 5.31 | 194.32 | 0.3653 | 959.2 | 999999 | |
| 11.24 | -3.00 | 6.12 | -3.00 | -16.59 | 149.04 | 5.29 | 192.35 | 0.4149 | -1121.3 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.45 | -19.83 | 148.33 | 4.58 | 189.38 | 0.4629 | -646.0 | -527.6 | |
| 0.00 | 1.34 | 0.00 | 0.72 | -16.14 | 147.77 | 4.02 | 189.63 | 0.4041 | -973.0 | -767.5 | |
| 0.00 | 0.71 | 0.00 | 0.38 | -14.83 | 147.75 | 3.99 | 190.16 | 0.3833 | -824.0 | -644.9 | |
| 0.00 | 1.07 | 0.00 | 0.57 | -14.11 | 147.45 | 3.70 | 189.75 | 0.3710 | 799.0 | 658.4 | |
| 0.00 | 1.34 | 0.00 | 0.72 | -15.42 | 147.19 | 3.44 | 188.54 | 0.3911 | -1025.0 | -730.5 | |
| 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. | |