SDO HMI 2014-04-11 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.76 | 0.00 | 9.96 | -13.37 | 304.46 | 3.48 | 206.87 | 0.1843 | 393.2 | 126.9 | |
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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 | 0.62 | 0.00 | 0.31 | -10.79 | 313.45 | 12.46 | 247.44 | 0.2305 | 837.0 | 663.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -14.28 | 311.40 | 10.41 | 229.86 | 0.2302 | 700.0 | 581.1 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -14.98 | 311.18 | 10.19 | 226.94 | 0.2351 | 922.0 | 810.1 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -14.10 | 310.89 | 9.90 | 229.08 | 0.2217 | 693.0 | 596.6 | |
| 0.00 | 1.76 | 0.00 | 0.89 | -12.17 | 310.75 | 9.76 | 236.19 | 0.2005 | 864.0 | 781.2 | |
| 0.00 | 1.50 | 0.00 | 0.76 | -12.47 | 310.70 | 9.71 | 234.78 | 0.2026 | 867.0 | 766.5 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -12.20 | 310.53 | 9.55 | 235.47 | 0.1977 | 829.0 | 668.8 | |
| 0.00 | 2.29 | 0.00 | 1.14 | -4.73 | 305.89 | 4.91 | 282.92 | 0.0879 | 723.0 | 563.6 | |
| 0.00 | 1.15 | 0.00 | 0.58 | -16.70 | 300.93 | -0.06 | 179.71 | 0.1887 | -785.0 | -632.8 | |
| 0.00 | 4.85 | 0.00 | 2.43 | -13.38 | 298.40 | -2.58 | 161.45 | 0.1385 | -949.0 | -773.5 | |
| 0.00 | 1.50 | 0.00 | 0.77 | -20.88 | 297.83 | -3.15 | 168.79 | 0.2653 | 750.0 | 501.9 | |
| 0.00 | 1.68 | 0.00 | 0.85 | -17.38 | 295.73 | -5.26 | 156.37 | 0.2191 | -732.0 | -584.1 | |
| 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. | |