SDO HMI 2014-10-16 20:00:30 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.80 | 0.00 | 8.57 | 14.52 | 356.98 | 21.13 | 298.86 | 0.3911 | -258.6 | -304.6 | |
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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 | 0.70 | 0.00 | 0.40 | 11.87 | 5.78 | 29.93 | 283.75 | 0.5048 | -617.0 | -578.8 | |
| 0.00 | 1.92 | 0.00 | 1.09 | 11.84 | 5.21 | 29.37 | 283.86 | 0.4964 | -801.0 | -612.4 | |
| 0.00 | 1.05 | 0.00 | 0.60 | 14.10 | 4.73 | 28.89 | 288.53 | 0.4962 | -697.0 | -614.6 | |
| 0.00 | 0.70 | 0.00 | 0.39 | 14.44 | 2.65 | 26.80 | 290.27 | 0.4675 | -584.0 | -494.5 | |
| 0.00 | 1.05 | 0.00 | 0.58 | 13.79 | 0.85 | 25.01 | 289.92 | 0.4386 | -651.0 | -556.3 | |
| 0.00 | 1.40 | 0.00 | 0.77 | 13.64 | 0.73 | 24.89 | 289.66 | 0.4362 | -775.0 | -550.2 | |
| 0.00 | 1.57 | 0.00 | 0.87 | 16.22 | 0.68 | 24.84 | 295.28 | 0.4480 | -697.0 | -596.8 | |
| 0.00 | 2.01 | 0.00 | 1.09 | 15.95 | 357.66 | 21.82 | 297.21 | 0.4036 | -803.0 | -719.1 | |
| 0.00 | 1.13 | 0.00 | 0.61 | 15.93 | 357.46 | 21.62 | 297.35 | 0.4006 | -983.0 | -817.8 | |
| 0.00 | 0.96 | 0.00 | 0.49 | 15.00 | 347.34 | 11.50 | 310.16 | 0.2532 | 792.0 | 613.5 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 15.46 | 343.69 | 7.85 | 322.15 | 0.2155 | 827.0 | 664.4 | |
| 0.00 | 0.96 | 0.00 | 0.48 | 14.48 | 342.66 | 6.82 | 322.95 | 0.1916 | 734.0 | 577.5 | |
| 0.00 | 1.22 | 0.00 | 0.62 | 15.64 | 341.70 | 5.86 | 330.27 | 0.1990 | 893.0 | 702.7 | |
| 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. | |