SDO HMI 2014-03-06 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.69 | 158.39 | 32.86 | 138.70 | -10.04 | 359.50 | -56.22 | 97.24 | 0.8269 | 605.3 | 302.8 | |
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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 | 1.21 | 0.00 | 1.00 | -14.82 | 1.95 | -53.77 | 103.11 | 0.8029 | 79.0 | 109.8 | |
| 0.00 | 1.30 | 0.00 | 1.07 | -13.93 | 1.85 | -53.87 | 101.99 | 0.8037 | 575.0 | 497.3 | |
| 0.00 | 2.42 | 0.00 | 2.02 | -9.52 | 1.62 | -54.11 | 96.51 | 0.8064 | -591.0 | -353.1 | |
| 14.09 | 124.06 | 12.12 | 106.97 | -9.60 | 0.28 | -55.44 | 96.66 | 0.8197 | 885.2 | 376.4 | |
| 18.24 | -4.00 | 15.80 | -4.00 | -10.32 | 359.99 | -55.73 | 97.55 | 0.8224 | 846.2 | 999999 | |
| 0.00 | 1.90 | 0.00 | 1.67 | -9.69 | 359.45 | -56.27 | 96.81 | 0.8279 | 479.0 | 327.3 | |
| 0.00 | 1.30 | 0.00 | 1.19 | -10.96 | 357.79 | -57.93 | 98.40 | 0.8431 | 374.0 | 288.5 | |
| 0.00 | 2.25 | 0.00 | 2.08 | -10.32 | 357.41 | -58.31 | 97.65 | 0.8468 | 479.0 | 355.6 | |
| 5.36 | 14.61 | 4.94 | 13.41 | -9.19 | 357.61 | -58.11 | 96.31 | 0.8454 | 417.7 | 341.7 | |
| 0.00 | 1.90 | 0.00 | 1.76 | -9.98 | 357.40 | -58.33 | 97.26 | 0.8470 | 109.0 | 54.0 | |
| 0.00 | 2.68 | 0.00 | 2.55 | -10.27 | 356.37 | -59.35 | 97.63 | 0.8562 | -490.0 | -421.8 | |
| 0.00 | 0.61 | 0.00 | 0.57 | -7.67 | 356.83 | -58.89 | 94.56 | 0.8533 | 472.0 | 412.6 | |
| 0.00 | 0.78 | 0.00 | 0.75 | -11.05 | 355.81 | -59.91 | 98.57 | 0.8609 | 357.0 | 292.0 | |
| 0.00 | 0.95 | 0.00 | 0.97 | -14.48 | 353.83 | -61.89 | 102.57 | 0.8770 | -251.0 | -295.4 | |
| 0.00 | 2.42 | 0.00 | 2.69 | -10.87 | 351.43 | -64.29 | 98.56 | 0.8967 | -600.0 | -503.8 | |
| 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. | |