SDO HMI 2014-10-02 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.25 | 0.00 | 10.66 | -5.01 | 138.91 | -29.87 | 110.64 | 0.5326 | -662.2 | -580.2 | |
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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 | 1.06 | 0.00 | 0.61 | -4.39 | 140.23 | -28.55 | 110.47 | 0.5107 | -881.0 | -821.8 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -4.49 | 139.68 | -29.11 | 110.25 | 0.5190 | -796.0 | -704.8 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -6.25 | 139.30 | -29.48 | 113.11 | 0.5340 | -809.0 | -678.6 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -4.05 | 139.21 | -29.57 | 109.16 | 0.5232 | -480.0 | -537.6 | |
| 0.00 | 2.82 | 0.00 | 1.65 | -5.93 | 139.01 | -29.77 | 112.34 | 0.5361 | -768.0 | -705.2 | |
| 0.00 | 1.50 | 0.00 | 0.88 | -6.52 | 138.97 | -29.81 | 113.32 | 0.5400 | -584.0 | -522.6 | |
| 0.00 | 1.41 | 0.00 | 0.82 | -3.21 | 139.07 | -29.71 | 107.53 | 0.5211 | -684.0 | -537.3 | |
| 0.00 | 1.59 | 0.00 | 0.93 | -5.51 | 138.93 | -29.85 | 111.55 | 0.5348 | -681.0 | -616.8 | |
| 0.00 | 2.38 | 0.00 | 1.38 | -4.10 | 138.93 | -29.85 | 109.06 | 0.5274 | -730.0 | -659.5 | |
| 0.00 | 2.47 | 0.00 | 1.44 | -3.63 | 138.64 | -30.14 | 108.03 | 0.5292 | -682.0 | -509.2 | |
| 0.00 | 1.94 | 0.00 | 1.16 | -6.71 | 137.41 | -31.37 | 112.53 | 0.5619 | -189.0 | -206.7 | |
| 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. | |