SDO HMI 2014-11-28 19:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.17 | 30.61 | 5.73 | 17.14 | 17.49 | 152.26 | 22.81 | 307.37 | 0.4671 | 334.4 | -49.4 | |
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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 | 0.77 | 0.00 | 0.45 | 21.41 | 154.96 | 25.51 | 310.89 | 0.5326 | 497.0 | 412.2 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 18.04 | 154.04 | 24.59 | 306.38 | 0.4935 | 649.0 | 487.4 | |
| 7.01 | 9.75 | 3.98 | 5.53 | 17.77 | 153.86 | 24.41 | 306.08 | 0.4891 | 995.3 | 619.2 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 17.89 | 153.54 | 24.09 | 306.64 | 0.4861 | 286.0 | 354.3 | |
| 0.00 | 0.85 | 0.00 | 0.48 | 17.84 | 152.61 | 23.17 | 307.55 | 0.4744 | 754.0 | 564.6 | |
| 0.00 | 1.97 | 0.00 | 1.10 | 16.86 | 152.25 | 22.80 | 306.19 | 0.4615 | 741.0 | 578.2 | |
| 0.94 | 1.97 | 0.52 | 1.09 | 15.72 | 152.04 | 22.59 | 304.30 | 0.4496 | 771.1 | 608.8 | |
| 0.51 | 1.45 | 0.28 | 0.80 | 15.57 | 151.92 | 22.48 | 304.14 | 0.4468 | 831.3 | 765.4 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 16.31 | 151.58 | 22.13 | 305.94 | 0.4485 | -592.0 | -514.1 | |
| 0.00 | 2.65 | 0.00 | 1.46 | 16.35 | 150.45 | 21.01 | 307.36 | 0.4346 | -926.0 | -843.2 | |
| 1.71 | 6.67 | 0.95 | 3.70 | 18.14 | 150.50 | 21.06 | 310.59 | 0.4516 | -920.0 | -643.1 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 17.40 | 149.72 | 20.27 | 310.28 | 0.4352 | -1036.0 | -754.6 | |
| 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. | |