SDO HMI 2014-04-05 21:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.10 | 0.00 | 9.23 | 5.39 | 24.81 | 5.19 | 336.03 | 0.2342 | 106.5 | -61.4 | |
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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 | 4.04 | 0.00 | 2.06 | 3.55 | 29.10 | 9.47 | 315.87 | 0.2370 | -925.0 | -739.3 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 3.45 | 28.18 | 8.56 | 318.48 | 0.2251 | -834.0 | -616.2 | |
| 0.00 | 1.67 | 0.00 | 0.84 | 2.09 | 26.66 | 7.03 | 319.80 | 0.1904 | -734.0 | -652.0 | |
| 0.00 | 1.49 | 0.00 | 0.76 | 4.27 | 26.22 | 6.60 | 327.87 | 0.2164 | -802.0 | -684.5 | |
| 0.00 | 1.41 | 0.00 | 0.71 | 4.00 | 26.22 | 6.60 | 327.20 | 0.2124 | -841.0 | -667.3 | |
| 0.00 | 1.58 | 0.00 | 0.81 | 7.60 | 24.90 | 5.27 | 339.18 | 0.2574 | 908.0 | 742.7 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 9.93 | 24.93 | 5.31 | 341.89 | 0.2946 | 686.0 | 571.4 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 7.91 | 24.57 | 4.94 | 340.78 | 0.2604 | 811.0 | 652.9 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 8.80 | 23.48 | 3.86 | 345.64 | 0.2696 | 575.0 | 509.7 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 5.44 | 17.58 | -2.05 | 9.93 | 0.2071 | 729.0 | 630.5 | |
| 0.00 | 1.93 | 0.00 | 0.98 | 5.71 | 17.55 | -2.08 | 9.85 | 0.2118 | 856.0 | 584.6 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 7.29 | 17.03 | -2.60 | 10.85 | 0.2398 | 849.0 | 723.5 | |
| 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. | |