SDO HMI 2011-11-26 12:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.49 | 63.99 | 16.58 | 33.58 | 17.63 | 214.47 | -10.52 | 31.73 | 0.3306 | 491.8 | 253.8 | |
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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 | 0.58 | 17.45 | 218.36 | -6.63 | 21.84 | 0.2977 | 781.0 | 537.6 | |
| 0.00 | 1.80 | 0.00 | 0.93 | 17.91 | 218.06 | -6.93 | 22.11 | 0.3066 | 892.0 | 662.0 | |
| 0.00 | 1.28 | 0.00 | 0.67 | 17.94 | 217.87 | -7.12 | 22.61 | 0.3083 | 804.0 | 698.9 | |
| 0.00 | 3.51 | 0.00 | 1.82 | 17.54 | 217.76 | -7.23 | 23.46 | 0.3029 | 856.0 | 848.0 | |
| 6.76 | 10.18 | 3.51 | 5.29 | 16.86 | 216.70 | -8.30 | 27.50 | 0.3004 | -1005.5 | -518.8 | |
| 0.00 | 3.85 | 0.00 | 2.00 | 16.89 | 216.32 | -8.67 | 28.50 | 0.3038 | -937.0 | -799.5 | |
| 0.00 | 2.22 | 0.00 | 1.17 | 18.21 | 215.56 | -9.43 | 28.39 | 0.3288 | -1035.0 | -831.2 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 16.55 | 215.62 | -9.38 | 30.98 | 0.3047 | -775.0 | -780.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.37 | 213.53 | -11.47 | 34.70 | 0.3348 | 937.0 | 666.5 | |
| 2.48 | 32.26 | 1.31 | 17.04 | 18.02 | 213.27 | -11.73 | 34.16 | 0.3458 | 1005.9 | 774.1 | |
| 0.00 | 2.48 | 0.00 | 1.31 | 17.62 | 213.26 | -11.74 | 34.87 | 0.3406 | 1046.0 | 910.4 | |
| 0.00 | 2.22 | 0.00 | 1.16 | 16.51 | 213.30 | -11.70 | 36.82 | 0.3257 | 810.0 | 643.8 | |
| 22.25 | -10.00 | 11.76 | -10.00 | 18.05 | 212.79 | -12.21 | 35.17 | 0.3507 | 1012.4 | 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. | |