SDO HMI 2011-05-02 12:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.03 | 0.00 | 9.94 | 13.78 | 112.63 | 19.28 | 313.39 | 0.4425 | -740.6 | -621.6 | |
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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 | 1.07 | 0.00 | 0.61 | 14.05 | 117.35 | 23.99 | 307.68 | 0.5004 | -735.0 | -573.8 | |
| 0.00 | 2.14 | 0.00 | 1.20 | 14.71 | 113.64 | 20.29 | 313.41 | 0.4636 | -816.0 | -660.7 | |
| 0.00 | 1.43 | 0.00 | 0.79 | 14.51 | 113.36 | 20.00 | 313.49 | 0.4583 | -819.0 | -684.8 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 14.31 | 113.00 | 19.65 | 313.66 | 0.4523 | -796.0 | -610.4 | |
| 0.00 | 3.66 | 0.00 | 2.02 | 13.76 | 112.79 | 19.44 | 313.06 | 0.4442 | -681.0 | -659.7 | |
| 0.00 | 1.16 | 0.00 | 0.64 | 14.07 | 112.46 | 19.10 | 314.07 | 0.4436 | -548.0 | -388.7 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 15.90 | 112.53 | 19.17 | 316.88 | 0.4640 | -816.0 | -647.3 | |
| 0.00 | 2.77 | 0.00 | 1.52 | 13.78 | 112.27 | 18.91 | 313.86 | 0.4384 | -828.0 | -736.1 | |
| 0.00 | 1.61 | 0.00 | 0.88 | 13.46 | 112.17 | 18.82 | 313.45 | 0.4340 | -696.0 | -445.0 | |
| 0.00 | 1.25 | 0.00 | 0.67 | 11.03 | 110.28 | 16.93 | 311.98 | 0.3861 | -786.0 | -638.4 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 10.12 | 106.76 | 13.41 | 316.78 | 0.3348 | -626.0 | -536.4 | |
| 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. | |