SDO HMI 2014-04-06 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.60 | 0.00 | 9.35 | -15.34 | 350.60 | -18.58 | 118.25 | 0.3516 | -820.0 | -667.2 | |
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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 | 1.14 | 0.00 | 0.59 | -17.22 | 356.63 | -12.56 | 132.96 | 0.2850 | -829.0 | -676.3 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -11.47 | 354.63 | -14.55 | 111.08 | 0.2651 | -900.0 | -684.8 | |
| 0.00 | 1.50 | 0.00 | 0.78 | -15.86 | 353.51 | -15.68 | 123.38 | 0.3127 | -945.0 | -747.9 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -15.76 | 353.32 | -15.87 | 122.83 | 0.3145 | -883.0 | -782.2 | |
| 0.00 | 2.29 | 0.00 | 1.20 | -15.74 | 352.80 | -16.39 | 122.01 | 0.3216 | -993.0 | -789.7 | |
| 0.00 | 1.14 | 0.00 | 0.60 | -9.99 | 350.64 | -18.55 | 102.82 | 0.3227 | -821.0 | -682.1 | |
| 0.00 | 0.70 | 0.00 | 0.38 | -15.99 | 349.17 | -20.02 | 118.13 | 0.3748 | -913.0 | -797.2 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -12.64 | 349.09 | -20.10 | 109.44 | 0.3572 | -813.0 | -634.6 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -20.28 | 348.06 | -21.13 | 126.45 | 0.4222 | -789.0 | -577.2 | |
| 0.00 | 1.94 | 0.00 | 1.04 | -15.78 | 348.52 | -20.66 | 116.97 | 0.3827 | -757.0 | -618.2 | |
| 0.00 | 3.25 | 0.00 | 1.75 | -15.52 | 348.12 | -21.07 | 115.96 | 0.3869 | -519.0 | -567.0 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -17.47 | 345.09 | -24.09 | 117.67 | 0.4415 | -678.0 | -547.0 | |
| 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. | |