SDO HMI 2014-11-11 07:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.71 | 0.00 | 10.30 | -9.99 | 338.14 | -21.98 | 121.58 | 0.4338 | -7.7 | -151.3 | |
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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 | 0.78 | 0.00 | 0.41 | -5.99 | 343.33 | -16.79 | 118.94 | 0.3297 | 734.0 | 560.8 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -9.14 | 343.07 | -17.05 | 126.32 | 0.3608 | 894.0 | 643.3 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -9.78 | 342.91 | -17.21 | 127.49 | 0.3690 | 861.0 | 710.9 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -8.69 | 342.43 | -17.68 | 124.32 | 0.3652 | 789.0 | 562.8 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -7.05 | 341.03 | -19.09 | 118.53 | 0.3711 | 721.0 | 522.4 | |
| 0.00 | 1.29 | 0.00 | 0.69 | -6.76 | 340.75 | -19.36 | 117.48 | 0.3728 | 765.0 | 573.6 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -11.09 | 339.86 | -20.26 | 125.78 | 0.4206 | 799.0 | 630.9 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -12.28 | 337.05 | -23.07 | 124.59 | 0.4669 | -378.0 | -436.4 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -12.20 | 336.70 | -23.42 | 124.04 | 0.4708 | -693.0 | -614.4 | |
| 0.00 | 1.03 | 0.00 | 0.57 | -9.78 | 336.57 | -23.54 | 119.36 | 0.4536 | -781.0 | -595.6 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -12.18 | 336.27 | -23.85 | 123.53 | 0.4761 | -727.0 | -494.2 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -10.21 | 336.38 | -23.74 | 119.99 | 0.4594 | -947.0 | -824.2 | |
| 0.00 | 2.59 | 0.00 | 1.44 | -10.00 | 336.26 | -23.86 | 119.47 | 0.4594 | -751.0 | -738.4 | |
| 0.00 | 1.81 | 0.00 | 1.03 | -10.87 | 334.52 | -25.60 | 119.40 | 0.4890 | -725.0 | -556.8 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -10.06 | 333.99 | -26.13 | 117.43 | 0.4905 | -677.0 | -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. | |