SDO HMI 2014-08-02 05:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.42 | 92.55 | 27.23 | 300.50 | 9.31 | 172.51 | -82.06 | 81.44 | 0.9884 | 17.8 | 92.3 | |
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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 | 1.09 | 0.00 | 1.84 | 7.93 | 180.95 | -73.62 | 83.47 | 0.9577 | -386.0 | -352.3 | |
| 4.26 | 13.85 | 8.47 | 27.55 | 10.29 | 178.19 | -76.38 | 80.85 | 0.9697 | -542.0 | -400.3 | |
| 0.00 | 1.09 | 0.00 | 2.62 | 10.65 | 175.50 | -79.07 | 80.31 | 0.9798 | 347.0 | 247.6 | |
| 0.00 | 1.00 | 0.00 | 2.49 | 10.15 | 175.15 | -79.42 | 80.79 | 0.9811 | 370.0 | 343.5 | |
| 0.00 | 0.27 | 0.00 | 0.67 | 9.89 | 175.39 | -79.18 | 81.07 | 0.9804 | 169.0 | 222.0 | |
| 0.00 | 3.08 | 0.00 | 8.69 | 10.97 | 173.69 | -80.88 | 79.86 | 0.9855 | 396.0 | 357.1 | |
| 0.00 | 3.17 | 0.00 | 8.81 | 10.56 | 173.98 | -80.59 | 80.29 | 0.9847 | 422.0 | 362.4 | |
| 0.00 | 1.00 | 0.00 | 2.66 | 9.64 | 174.39 | -80.18 | 81.26 | 0.9837 | 274.0 | 267.1 | |
| 0.00 | 1.18 | 0.00 | 4.06 | 11.29 | 171.90 | -82.67 | 79.41 | 0.9901 | 169.0 | 205.5 | |
| 1.27 | 66.82 | 4.30 | 241.11 | 8.68 | 172.28 | -82.29 | 82.06 | 0.9897 | 345.1 | 108.0 | |
| 3.89 | -10.00 | 14.46 | -10.00 | 9.15 | 171.43 | -83.14 | 81.52 | 0.9916 | 136.5 | 999999 | |
| 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. | |