SDO HMI 2011-02-12 21:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.60 | 128.28 | 27.70 | 73.15 | 19.77 | 63.90 | 13.64 | 333.40 | 0.4978 | 294.1 | 159.3 | |
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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 | 1.54 | 0.00 | 0.90 | 21.18 | 66.30 | 16.04 | 330.94 | 0.5326 | -596.0 | -491.1 | |
| 0.00 | 2.65 | 0.00 | 1.53 | 19.71 | 66.11 | 15.85 | 329.75 | 0.5125 | -601.0 | -509.0 | |
| 13.35 | 28.33 | 7.65 | 16.20 | 19.28 | 65.90 | 15.64 | 329.62 | 0.5054 | -981.2 | -710.8 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 19.90 | 65.90 | 15.64 | 330.28 | 0.5134 | -591.0 | -392.1 | |
| 0.00 | 0.86 | 0.00 | 0.49 | 20.24 | 65.18 | 14.92 | 331.75 | 0.5126 | -667.0 | -598.7 | |
| 0.00 | 1.80 | 0.00 | 1.02 | 19.02 | 64.13 | 13.87 | 332.27 | 0.4891 | 576.0 | 547.3 | |
| 2.48 | 81.38 | 1.42 | 46.33 | 20.47 | 63.83 | 13.58 | 334.14 | 0.5064 | 419.8 | 405.0 | |
| 2.22 | -7.00 | 1.27 | -7.00 | 20.39 | 63.57 | 13.31 | 334.52 | 0.5037 | 603.9 | 999999 | |
| 5.39 | -7.00 | 3.05 | -7.00 | 19.33 | 63.35 | 13.09 | 333.90 | 0.4878 | 990.1 | 999999 | |
| 6.93 | -7.00 | 3.96 | -7.00 | 20.12 | 63.35 | 13.09 | 334.64 | 0.4986 | 806.1 | 999999 | |
| 15.83 | -7.00 | 8.99 | -7.00 | 19.75 | 62.96 | 12.71 | 334.95 | 0.4910 | 1033.2 | 999999 | |
| 0.43 | 9.33 | 0.24 | 5.31 | 20.37 | 62.63 | 12.37 | 336.08 | 0.4974 | 864.4 | 754.7 | |
| 1.97 | -12.00 | 1.12 | -12.00 | 20.16 | 62.45 | 12.19 | 336.21 | 0.4935 | 810.3 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 20.35 | 61.98 | 11.72 | 337.18 | 0.4933 | 747.0 | 620.3 | |
| 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. | |