SDO HMI 2014-03-28 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 | 11.13 | 0.00 | 6.99 | -22.81 | 98.56 | -35.39 | 119.35 | 0.6099 | 557.8 | 446.5 | |
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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 | 1.49 | 0.00 | 0.88 | -22.23 | 103.59 | -30.36 | 121.07 | 0.5484 | 714.0 | 493.4 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -22.22 | 102.91 | -31.04 | 120.61 | 0.5568 | 819.0 | 614.6 | |
| 0.00 | 1.84 | 0.00 | 1.10 | -21.99 | 102.74 | -31.21 | 120.12 | 0.5576 | 731.0 | 634.9 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -22.39 | 102.49 | -31.46 | 120.62 | 0.5629 | 601.0 | 471.7 | |
| 0.00 | 0.88 | 0.00 | 0.53 | -22.95 | 101.50 | -32.45 | 120.93 | 0.5782 | 726.0 | 495.2 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -21.71 | 100.21 | -33.74 | 118.20 | 0.5877 | 614.0 | 442.6 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -21.55 | 100.02 | -33.93 | 117.83 | 0.5893 | 638.0 | 545.0 | |
| 0.00 | 1.31 | 0.00 | 0.81 | -21.61 | 99.11 | -34.85 | 117.47 | 0.6009 | 659.0 | 550.6 | |
| 0.00 | 1.14 | 0.00 | 0.78 | -23.03 | 92.10 | -41.85 | 116.64 | 0.6893 | 642.0 | 480.0 | |
| 0.00 | 0.61 | 0.00 | 0.44 | -26.07 | 89.71 | -44.25 | 119.93 | 0.7255 | 573.0 | 420.3 | |
| 0.00 | 0.70 | 0.00 | 0.55 | -26.91 | 84.54 | -49.41 | 119.38 | 0.7794 | -581.0 | -485.9 | |
| 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. | |