SDO HMI 2014-09-20 00:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.66 | 18.98 | 1.60 | 11.38 | -21.24 | 310.36 | -19.54 | 146.41 | 0.5648 | -267.5 | -287.6 | |
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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 | 0.27 | 0.00 | 0.15 | -19.30 | 313.83 | -16.07 | 149.34 | 0.5142 | 689.0 | 703.7 | |
| 0.00 | 1.95 | 0.00 | 1.12 | -18.91 | 313.51 | -16.39 | 148.42 | 0.5118 | 937.0 | 727.2 | |
| 0.00 | 1.42 | 0.00 | 0.83 | -19.95 | 312.73 | -17.17 | 148.34 | 0.5308 | 605.0 | 455.2 | |
| 0.53 | 1.33 | 0.32 | 0.80 | -21.79 | 310.28 | -19.62 | 146.82 | 0.5719 | -885.8 | -844.3 | |
| 0.00 | 1.33 | 0.00 | 0.80 | -21.87 | 310.03 | -19.87 | 146.57 | 0.5748 | -557.0 | -423.7 | |
| 0.00 | 1.24 | 0.00 | 0.75 | -21.52 | 310.05 | -19.85 | 146.24 | 0.5707 | -349.0 | -519.6 | |
| 0.80 | 2.84 | 0.48 | 1.70 | -21.04 | 310.08 | -19.82 | 145.78 | 0.5649 | -436.9 | -348.9 | |
| 0.00 | 1.24 | 0.00 | 0.76 | -22.27 | 309.55 | -20.35 | 146.37 | 0.5831 | -390.0 | -467.6 | |
| 0.00 | 2.48 | 0.00 | 1.51 | -22.03 | 309.45 | -20.45 | 145.99 | 0.5812 | -754.0 | -511.0 | |
| 1.33 | 2.84 | 0.80 | 1.72 | -21.65 | 309.44 | -20.46 | 145.58 | 0.5770 | -906.7 | -734.1 | |
| 0.00 | 2.04 | 0.00 | 1.24 | -21.63 | 309.20 | -20.70 | 145.25 | 0.5787 | -743.0 | -612.3 | |
| 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. | |