SDO HMI 2014-04-01 11:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.11 | 0.00 | 10.75 | -27.65 | 78.88 | 0.97 | 181.32 | 0.3776 | -515.2 | -428.1 | |
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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 | 1.32 | 0.00 | 0.73 | -28.42 | 93.96 | 16.05 | 212.82 | 0.4504 | 585.0 | 451.2 | |
| 0.00 | 1.93 | 0.00 | 1.05 | -26.45 | 91.80 | 13.89 | 212.00 | 0.4073 | 828.0 | 690.8 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -27.30 | 83.11 | 5.20 | 192.77 | 0.3659 | -739.0 | -539.5 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -29.13 | 79.45 | 1.54 | 183.50 | 0.3869 | -832.0 | -706.3 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -29.29 | 79.21 | 1.30 | 182.93 | 0.3893 | -710.0 | -527.2 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -29.22 | 78.01 | 0.10 | 180.23 | 0.3877 | -742.0 | -612.6 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -33.79 | 76.82 | -1.09 | 178.02 | 0.4604 | -722.0 | -519.6 | |
| 0.00 | 2.90 | 0.00 | 1.55 | -28.90 | 76.37 | -1.54 | 176.46 | 0.3831 | -951.0 | -776.4 | |
| 0.00 | 1.67 | 0.00 | 0.88 | -27.03 | 75.99 | -1.92 | 175.14 | 0.3532 | -890.0 | -626.2 | |
| 0.00 | 1.49 | 0.00 | 0.78 | -25.34 | 75.59 | -2.32 | 173.54 | 0.3262 | -637.0 | -440.8 | |
| 0.00 | 4.65 | 0.00 | 2.45 | -25.24 | 71.94 | -5.97 | 163.70 | 0.3365 | -857.0 | -662.0 | |
| 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. | |