SDO HMI 2014-12-05 00:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.57 | 0.00 | 6.13 | 13.74 | 19.28 | -28.33 | 63.25 | 0.5186 | -671.3 | -533.2 | |
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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 | 0.68 | 0.00 | 0.38 | 15.20 | 24.24 | -23.37 | 56.23 | 0.4624 | -823.0 | -546.8 | |
| 0.00 | 1.62 | 0.00 | 0.91 | 15.11 | 23.75 | -23.86 | 56.92 | 0.4680 | -610.0 | -484.3 | |
| 0.00 | 1.02 | 0.00 | 0.57 | 8.26 | 21.00 | -26.61 | 72.78 | 0.4660 | -716.0 | -560.8 | |
| 0.00 | 1.62 | 0.00 | 0.94 | 14.46 | 19.23 | -28.38 | 62.10 | 0.5229 | -772.0 | -610.3 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 14.31 | 18.59 | -29.02 | 62.84 | 0.5304 | -562.0 | -436.6 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 13.64 | 18.47 | -29.14 | 64.10 | 0.5281 | -744.0 | -557.4 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 13.70 | 18.22 | -29.39 | 64.17 | 0.5318 | -704.0 | -560.3 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 10.74 | 17.12 | -30.49 | 70.11 | 0.5322 | -658.0 | -552.5 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 15.47 | 16.25 | -31.36 | 62.53 | 0.5675 | -457.0 | -408.7 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 13.21 | 16.49 | -31.12 | 66.13 | 0.5523 | -635.0 | -539.3 | |
| 0.00 | 1.19 | 0.00 | 0.72 | 15.34 | 15.51 | -32.09 | 63.21 | 0.5762 | -703.0 | -553.3 | |
| 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. | |