SDO HMI 2014-10-01 22:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.54 | 0.00 | 10.04 | -5.00 | 139.32 | -33.31 | 108.54 | 0.5793 | -716.3 | -646.5 | |
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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 | 2.29 | 0.00 | 1.37 | -4.27 | 140.10 | -32.53 | 107.79 | 0.5653 | -890.0 | -754.5 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -3.92 | 139.94 | -32.69 | 107.10 | 0.5659 | -757.0 | -621.4 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -4.97 | 139.74 | -32.89 | 108.74 | 0.5735 | -873.0 | -722.0 | |
| 0.00 | 2.20 | 0.00 | 1.32 | -4.08 | 139.79 | -32.84 | 107.29 | 0.5687 | -600.0 | -622.8 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -4.45 | 139.66 | -32.97 | 107.85 | 0.5721 | -565.0 | -561.2 | |
| 0.00 | 0.53 | 0.00 | 0.32 | -4.96 | 139.35 | -33.28 | 108.51 | 0.5788 | -782.0 | -675.3 | |
| 0.00 | 1.67 | 0.00 | 1.02 | -5.10 | 139.16 | -33.47 | 108.62 | 0.5819 | -665.0 | -534.1 | |
| 0.00 | 2.55 | 0.00 | 1.56 | -6.39 | 139.07 | -33.56 | 110.66 | 0.5894 | -737.0 | -717.8 | |
| 0.00 | 1.06 | 0.00 | 0.64 | -3.94 | 139.11 | -33.52 | 106.69 | 0.5773 | -812.0 | -684.2 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -5.94 | 138.89 | -33.75 | 109.83 | 0.5896 | -732.0 | -631.2 | |
| 0.00 | 1.23 | 0.00 | 0.75 | -5.52 | 138.77 | -33.86 | 109.09 | 0.5891 | -685.0 | -589.5 | |
| 0.00 | 0.44 | 0.00 | 0.27 | -4.11 | 138.78 | -33.85 | 106.81 | 0.5826 | -545.0 | -502.8 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -7.20 | 137.09 | -35.54 | 110.76 | 0.6191 | -669.0 | -549.3 | |
| 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. | |