SDO HMI 2014-03-25 05:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.11 | 0.00 | 8.67 | -13.46 | 132.17 | -41.34 | 102.28 | 0.6606 | 553.9 | 466.4 | |
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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 | 0.61 | 0.00 | 0.36 | -10.68 | 140.02 | -33.49 | 99.00 | 0.5512 | 602.0 | 514.0 | |
| 0.00 | 1.14 | 0.00 | 0.69 | -7.05 | 138.25 | -35.27 | 92.48 | 0.5758 | 565.0 | 441.5 | |
| 0.00 | 1.05 | 0.00 | 0.65 | -6.32 | 136.40 | -37.11 | 91.37 | 0.6021 | 684.0 | 561.6 | |
| 0.00 | 0.79 | 0.00 | 0.49 | -6.60 | 136.23 | -37.29 | 91.86 | 0.6044 | 594.0 | 491.4 | |
| 0.00 | 1.22 | 0.00 | 0.81 | -14.79 | 131.97 | -41.55 | 104.58 | 0.6650 | 837.0 | 715.1 | |
| 0.00 | 0.96 | 0.00 | 0.63 | -14.43 | 132.05 | -41.47 | 104.05 | 0.6634 | 688.0 | 550.8 | |
| 0.00 | 0.70 | 0.00 | 0.47 | -15.11 | 131.43 | -42.09 | 104.97 | 0.6721 | 466.0 | 452.0 | |
| 0.00 | 0.87 | 0.00 | 0.59 | -15.21 | 131.15 | -42.36 | 105.08 | 0.6757 | 580.0 | 443.3 | |
| 0.00 | 1.31 | 0.00 | 0.88 | -15.02 | 131.07 | -42.44 | 104.78 | 0.6764 | 490.0 | 425.5 | |
| 0.00 | 1.14 | 0.00 | 0.77 | -15.42 | 130.68 | -42.84 | 105.30 | 0.6819 | 523.0 | 406.1 | |
| 0.00 | 0.70 | 0.00 | 0.48 | -15.82 | 130.32 | -43.20 | 105.82 | 0.6869 | 329.0 | 333.9 | |
| 0.00 | 0.96 | 0.00 | 0.68 | -18.87 | 128.19 | -45.33 | 109.74 | 0.7172 | 530.0 | 357.5 | |
| 0.00 | 0.96 | 0.00 | 0.66 | -13.17 | 129.22 | -44.30 | 101.85 | 0.6972 | 494.0 | 467.6 | |
| 0.00 | 0.70 | 0.00 | 0.51 | -18.26 | 126.48 | -47.03 | 108.58 | 0.7354 | 372.0 | 289.0 | |
| 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. | |