SDO HMI 2011-11-26 06:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.10 | 63.60 | 17.10 | 33.79 | 17.76 | 214.53 | -13.74 | 38.68 | 0.3623 | 245.6 | 20.1 | |
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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 | 3.25 | 0.00 | 1.70 | 17.10 | 218.27 | -10.00 | 31.69 | 0.3175 | 917.0 | 655.8 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 17.50 | 218.22 | -10.06 | 31.14 | 0.3235 | 849.0 | 682.9 | |
| 0.00 | 0.68 | 0.00 | 0.36 | 18.39 | 217.59 | -10.68 | 31.17 | 0.3412 | 805.0 | 594.0 | |
| 0.00 | 1.37 | 0.00 | 0.73 | 19.20 | 217.10 | -11.18 | 31.05 | 0.3565 | 790.0 | 677.4 | |
| 9.07 | 10.70 | 4.76 | 5.62 | 17.00 | 216.45 | -11.83 | 36.24 | 0.3330 | -991.5 | -731.5 | |
| 0.00 | 2.14 | 0.00 | 1.13 | 17.00 | 216.07 | -12.20 | 37.09 | 0.3367 | -625.0 | -460.0 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 17.58 | 215.84 | -12.43 | 36.52 | 0.3465 | -582.0 | -472.4 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 16.63 | 215.52 | -12.75 | 38.99 | 0.3376 | -817.0 | -706.4 | |
| 0.00 | 4.45 | 0.00 | 2.36 | 18.20 | 215.38 | -12.89 | 36.40 | 0.3588 | -1087.0 | -771.1 | |
| 0.00 | 1.20 | 0.00 | 0.63 | 17.58 | 215.36 | -12.91 | 37.54 | 0.3512 | -892.0 | -730.2 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 17.33 | 215.32 | -12.96 | 38.09 | 0.3485 | -968.0 | -679.6 | |
| 0.00 | 2.65 | 0.00 | 1.41 | 17.98 | 215.24 | -13.04 | 37.08 | 0.3575 | -763.0 | -543.6 | |
| 0.00 | 1.88 | 0.00 | 1.00 | 17.88 | 213.51 | -14.76 | 40.65 | 0.3738 | 1007.0 | 889.0 | |
| 23.03 | 28.94 | 12.34 | 15.50 | 17.96 | 212.76 | -15.51 | 41.85 | 0.3829 | 1075.8 | 716.2 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 20.41 | 211.67 | -16.60 | 39.51 | 0.4227 | 201.0 | 287.5 | |
| 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. | |