SDO HMI 2011-11-27 09:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.39 | 43.46 | 9.49 | 22.49 | 17.92 | 214.77 | 1.31 | 355.56 | 0.2892 | 460.6 | 524.7 | |
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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 | 3.59 | 0.00 | 1.86 | 17.80 | 218.45 | 4.99 | 343.68 | 0.2960 | 884.0 | 770.3 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.99 | 218.20 | 4.75 | 344.61 | 0.2978 | 738.0 | 687.9 | |
| 7.27 | 8.30 | 3.74 | 4.27 | 16.42 | 217.45 | 3.99 | 345.57 | 0.2692 | -973.0 | -851.7 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.82 | 216.57 | 3.12 | 351.32 | 0.3382 | 608.0 | 460.6 | |
| 0.00 | 1.03 | 0.00 | 0.54 | 20.35 | 216.34 | 2.89 | 351.74 | 0.3300 | 858.0 | 655.7 | |
| 0.00 | 1.28 | 0.00 | 0.68 | 21.14 | 216.29 | 2.84 | 352.22 | 0.3427 | 760.0 | 624.7 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 17.31 | 215.79 | 2.34 | 351.93 | 0.2785 | -727.0 | -552.1 | |
| 0.00 | 1.11 | 0.00 | 0.57 | 17.34 | 213.35 | -0.11 | 0.38 | 0.2763 | 927.0 | 693.5 | |
| 0.00 | 0.60 | 0.00 | 0.31 | 16.73 | 213.29 | -0.17 | 0.62 | 0.2659 | 886.0 | 683.1 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 18.02 | 213.25 | -0.20 | 0.68 | 0.2877 | 838.0 | 697.9 | |
| 0.00 | 2.99 | 0.00 | 1.55 | 17.68 | 213.22 | -0.23 | 0.80 | 0.2820 | 811.0 | 686.6 | |
| 11.12 | 18.65 | 5.75 | 9.64 | 18.05 | 212.94 | -0.51 | 1.71 | 0.2883 | 999.1 | 627.7 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 20.32 | 212.56 | -0.90 | 2.60 | 0.3264 | 749.0 | 598.2 | |
| 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. | |