SDO HMI 2014-03-29 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 | 15.23 | 0.00 | 9.40 | -11.75 | 84.30 | -36.47 | 100.59 | 0.5927 | 247.0 | 218.8 | |
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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 | 1.31 | 0.00 | 0.76 | -10.32 | 89.14 | -31.63 | 98.83 | 0.5242 | 867.0 | 686.8 | |
| 0.00 | 0.61 | 0.00 | 0.36 | -10.19 | 89.01 | -31.75 | 98.57 | 0.5259 | 542.0 | 551.3 | |
| 0.00 | 1.75 | 0.00 | 1.02 | -10.36 | 88.85 | -31.92 | 98.87 | 0.5285 | 671.0 | 469.8 | |
| 0.00 | 1.49 | 0.00 | 0.87 | -10.34 | 88.49 | -32.28 | 98.78 | 0.5337 | 784.0 | 612.8 | |
| 0.00 | 2.80 | 0.00 | 1.65 | -9.92 | 87.63 | -33.13 | 97.92 | 0.5457 | 758.0 | 633.2 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -12.36 | 84.39 | -36.37 | 101.78 | 0.5940 | 730.0 | 604.4 | |
| 0.00 | 1.66 | 0.00 | 1.03 | -11.69 | 83.89 | -36.88 | 100.59 | 0.6001 | 404.0 | 439.7 | |
| 0.00 | 0.88 | 0.00 | 0.57 | -15.89 | 80.56 | -40.20 | 106.69 | 0.6504 | -532.0 | -439.0 | |
| 0.00 | 0.96 | 0.00 | 0.65 | -14.74 | 78.35 | -42.41 | 104.56 | 0.6762 | -676.0 | -564.5 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -15.14 | 77.92 | -42.85 | 105.07 | 0.6821 | -84.0 | -133.6 | |
| 0.00 | 1.93 | 0.00 | 1.30 | -12.07 | 77.94 | -42.82 | 100.56 | 0.6785 | -747.0 | -586.8 | |
| 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. | |