SDO HMI 2014-10-03 09:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.28 | 0.00 | 8.55 | -5.38 | 138.01 | -15.39 | 127.75 | 0.3353 | -833.3 | -662.0 | |
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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 | 1.41 | 0.00 | 0.73 | -3.96 | 139.97 | -13.43 | 127.87 | 0.2948 | -824.0 | -544.3 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -4.48 | 139.90 | -13.50 | 129.08 | 0.3012 | -851.0 | -702.2 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -5.65 | 139.81 | -13.59 | 131.78 | 0.3150 | -1075.0 | -843.4 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -6.05 | 138.68 | -14.72 | 130.42 | 0.3334 | -933.0 | -758.5 | |
| 0.00 | 2.46 | 0.00 | 1.30 | -6.32 | 138.67 | -14.73 | 131.03 | 0.3365 | -735.0 | -619.2 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -6.00 | 138.31 | -15.09 | 129.59 | 0.3375 | -755.0 | -536.0 | |
| 0.00 | 1.32 | 0.00 | 0.70 | -5.69 | 136.37 | -17.03 | 125.49 | 0.3595 | -769.0 | -588.9 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -5.44 | 136.34 | -17.06 | 124.90 | 0.3575 | -942.0 | -769.4 | |
| 0.00 | 1.50 | 0.00 | 0.79 | -5.29 | 136.25 | -17.15 | 124.41 | 0.3573 | -797.0 | -650.2 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -4.94 | 135.92 | -17.48 | 123.05 | 0.3586 | -745.0 | -685.3 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -4.69 | 135.89 | -17.51 | 122.44 | 0.3568 | -740.0 | -556.8 | |
| 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. | |