SDO HMI 2014-09-24 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 |
| 0.00 | 23.02 | 0.00 | 12.62 | -14.83 | 286.24 | 9.13 | 202.27 | 0.4249 | 723.5 | 565.8 | |
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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 | 2.57 | 0.00 | 1.42 | -4.41 | 300.75 | 23.65 | 244.83 | 0.4437 | 602.0 | 449.0 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -10.26 | 299.75 | 22.64 | 232.79 | 0.4776 | 511.0 | 496.8 | |
| 0.00 | 0.97 | 0.00 | 0.54 | -9.22 | 299.67 | 22.57 | 234.49 | 0.4673 | 831.0 | 655.8 | |
| 0.00 | 1.77 | 0.00 | 0.96 | -12.16 | 290.63 | 13.52 | 215.11 | 0.3992 | 789.0 | 569.4 | |
| 0.00 | 2.83 | 0.00 | 1.62 | -21.68 | 287.00 | 9.90 | 198.46 | 0.5065 | 762.0 | 528.8 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -23.01 | 282.64 | 5.54 | 190.07 | 0.5098 | 737.0 | 687.3 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -23.40 | 282.49 | 5.39 | 189.67 | 0.5151 | 705.0 | 579.5 | |
| 0.00 | 1.24 | 0.00 | 0.71 | -22.87 | 282.47 | 5.37 | 189.82 | 0.5073 | 778.0 | 550.6 | |
| 0.00 | 1.33 | 0.00 | 0.69 | -10.93 | 281.97 | 4.86 | 195.14 | 0.3201 | 888.0 | 666.9 | |
| 0.00 | 3.63 | 0.00 | 1.93 | -13.64 | 281.89 | 4.79 | 192.96 | 0.3631 | 752.0 | 583.9 | |
| 0.00 | 1.33 | 0.00 | 0.73 | -17.68 | 281.54 | 4.43 | 190.01 | 0.4257 | 674.0 | 577.9 | |
| 0.00 | 0.80 | 0.00 | 0.42 | -14.37 | 281.13 | 4.02 | 190.56 | 0.3722 | 670.0 | 535.2 | |
| 0.00 | 0.80 | 0.00 | 0.46 | -24.57 | 280.68 | 3.58 | 186.19 | 0.5287 | 729.0 | 548.9 | |
| 0.00 | 2.92 | 0.00 | 1.52 | -10.77 | 278.29 | 1.18 | 183.79 | 0.3075 | 701.0 | 596.9 | |
| 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. | |