SDO HMI 2011-11-10 04:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 84.15 | 156.89 | 47.61 | 88.97 | -25.14 | 85.33 | 5.05 | 189.36 | 0.4879 | -179.3 | -1.0 | |
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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 | 1.03 | 0.00 | 0.59 | -25.70 | 89.08 | 8.80 | 195.83 | 0.5076 | -641.0 | -487.2 | |
| 23.79 | 60.86 | 13.62 | 34.87 | -25.75 | 87.76 | 7.48 | 193.52 | 0.5033 | 1104.6 | 272.1 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -25.17 | 87.39 | 7.11 | 193.17 | 0.4935 | 1096.0 | 918.7 | |
| 0.00 | 1.29 | 0.00 | 0.73 | -24.76 | 87.23 | 6.95 | 193.10 | 0.4869 | 713.0 | 583.9 | |
| 5.52 | 6.55 | 3.10 | 3.68 | -24.09 | 86.31 | 6.03 | 191.73 | 0.4737 | 915.8 | 906.1 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -24.59 | 86.17 | 5.89 | 191.24 | 0.4809 | 537.0 | 432.7 | |
| 0.00 | 1.29 | 0.00 | 0.73 | -24.72 | 85.32 | 5.04 | 189.61 | 0.4805 | 853.0 | 595.1 | |
| 0.00 | 1.64 | 0.00 | 0.92 | -24.21 | 84.94 | 4.66 | 189.08 | 0.4718 | 787.0 | 518.2 | |
| 0.00 | 4.40 | 0.00 | 2.46 | -23.87 | 84.48 | 4.20 | 188.30 | 0.4656 | -615.0 | -312.6 | |
| 0.00 | 3.62 | 0.00 | 2.03 | -24.18 | 84.42 | 4.14 | 188.09 | 0.4701 | -206.0 | -137.7 | |
| 19.31 | 25.86 | 10.80 | 14.47 | -24.01 | 83.80 | 3.52 | 186.93 | 0.4662 | -1018.6 | -525.3 | |
| 1.47 | 41.72 | 0.83 | 23.63 | -25.76 | 83.42 | 3.14 | 185.77 | 0.4923 | -568.4 | -669.3 | |
| 18.71 | -12.00 | 10.59 | -12.00 | -25.38 | 83.05 | 2.77 | 185.17 | 0.4861 | -1023.9 | 999999 | |
| 5.26 | 6.90 | 2.96 | 3.88 | -24.88 | 82.84 | 2.56 | 184.88 | 0.4781 | -997.1 | -823.4 | |
| 10.09 | -12.00 | 5.71 | -12.00 | -25.45 | 82.55 | 2.27 | 184.24 | 0.4865 | -895.3 | 999999 | |
| 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. | |