SDO HMI 2014-08-02 08:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.88 | 102.85 | 23.48 | 289.43 | 9.16 | 172.47 | -80.46 | 81.71 | 0.9841 | 147.2 | 81.4 | |
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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 | 0.63 | 0.00 | 0.98 | 7.92 | 181.08 | -71.85 | 83.60 | 0.9485 | -404.0 | -394.1 | |
| 2.72 | 12.13 | 4.89 | 21.80 | 10.23 | 178.09 | -74.84 | 81.00 | 0.9629 | -552.3 | -436.7 | |
| 0.00 | 0.54 | 0.00 | 1.19 | 10.41 | 175.16 | -77.77 | 80.64 | 0.9752 | 389.0 | 357.5 | |
| 0.00 | 2.44 | 0.00 | 5.37 | 10.09 | 175.12 | -77.80 | 80.96 | 0.9754 | 435.0 | 379.5 | |
| 0.00 | 3.71 | 0.00 | 9.17 | 11.03 | 173.61 | -79.32 | 79.90 | 0.9806 | 601.0 | 431.7 | |
| 0.00 | 0.91 | 0.00 | 2.22 | 10.71 | 173.77 | -79.15 | 80.25 | 0.9801 | 484.0 | 441.8 | |
| 0.00 | 1.63 | 0.00 | 4.71 | 11.39 | 171.88 | -81.05 | 79.42 | 0.9859 | 306.0 | 221.0 | |
| 0.00 | 0.54 | 0.00 | 1.54 | 11.04 | 172.12 | -80.81 | 79.79 | 0.9852 | 413.0 | 405.0 | |
| 0.00 | 7.70 | 0.00 | 19.05 | 9.15 | 173.70 | -79.23 | 81.83 | 0.9807 | 518.0 | 428.0 | |
| 0.00 | 0.27 | 0.00 | 0.72 | 9.12 | 172.84 | -80.09 | 81.79 | 0.9835 | 522.0 | 470.7 | |
| 1.27 | 33.23 | 3.58 | 99.44 | 8.70 | 172.29 | -80.64 | 82.18 | 0.9853 | 388.1 | 139.6 | |
| 3.62 | 39.12 | 10.99 | 123.24 | 9.21 | 171.57 | -81.36 | 81.60 | 0.9872 | 289.8 | -8.7 | |
| 1.27 | -11.00 | 4.02 | -11.00 | 8.28 | 171.25 | -81.68 | 82.52 | 0.9883 | -88.6 | 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. | |