SDO HMI 2014-04-02 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.75 | 0.00 | 8.22 | -26.10 | 84.70 | 16.70 | 214.93 | 0.4514 | -57.4 | 10.0 | |
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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 | 2.11 | 0.00 | 1.26 | -21.67 | 99.59 | 31.59 | 240.32 | 0.5625 | 669.0 | 574.4 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -21.72 | 94.46 | 26.46 | 236.53 | 0.4983 | 692.0 | 595.0 | |
| 0.00 | 0.61 | 0.00 | 0.35 | -26.56 | 91.55 | 23.55 | 225.47 | 0.5034 | 606.0 | 581.4 | |
| 0.00 | 1.84 | 0.00 | 1.01 | -22.14 | 89.06 | 21.06 | 230.27 | 0.4346 | 742.0 | 661.8 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -27.08 | 89.73 | 21.73 | 222.57 | 0.4893 | 885.0 | 762.6 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -27.76 | 88.74 | 20.74 | 220.32 | 0.4863 | 613.0 | 495.3 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -26.22 | 82.59 | 14.59 | 213.55 | 0.4107 | -687.0 | -596.4 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -27.39 | 76.88 | 8.88 | 200.96 | 0.3850 | -651.0 | -568.2 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -28.69 | 76.33 | 8.33 | 198.55 | 0.4014 | -671.0 | -565.0 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -29.32 | 75.79 | 7.79 | 196.91 | 0.4082 | -879.0 | -742.9 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -27.55 | 74.68 | 6.68 | 195.98 | 0.3761 | -801.0 | -716.9 | |
| 0.00 | 0.79 | 0.00 | 0.42 | -26.45 | 71.86 | 3.86 | 190.00 | 0.3485 | -581.0 | -479.4 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -32.49 | 71.62 | 3.62 | 186.93 | 0.4436 | -683.0 | -647.0 | |
| 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. | |