SDO HMI 2011-07-01 14:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.89 | 40.59 | 7.10 | 20.77 | 15.97 | 23.85 | 5.47 | 337.49 | 0.2507 | 112.1 | -68.1 | |
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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 | 1.27 | 0.00 | 0.67 | 20.05 | 27.21 | 8.83 | 334.00 | 0.3305 | -688.0 | -641.9 | |
| 5.81 | 11.99 | 2.96 | 6.11 | 13.46 | 26.69 | 8.31 | 322.64 | 0.2326 | 1086.8 | 684.3 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 15.27 | 25.32 | 6.94 | 331.52 | 0.2455 | -845.0 | -648.9 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 15.68 | 25.27 | 6.89 | 332.49 | 0.2512 | -1036.0 | -763.7 | |
| 1.09 | 2.91 | 0.56 | 1.49 | 16.33 | 25.07 | 6.69 | 334.37 | 0.2595 | -1020.3 | -813.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 15.55 | 24.60 | 6.22 | 334.60 | 0.2443 | -1117.0 | -979.5 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 14.59 | 24.38 | 6.00 | 333.54 | 0.2280 | -807.0 | -573.5 | |
| 0.00 | 2.91 | 0.00 | 1.49 | 16.53 | 23.64 | 5.26 | 339.60 | 0.2531 | -1061.0 | -866.1 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 18.36 | 21.34 | 2.96 | 349.60 | 0.2727 | -647.0 | -529.2 | |
| 0.00 | 2.72 | 0.00 | 1.40 | 17.92 | 21.30 | 2.92 | 349.42 | 0.2652 | -334.0 | -74.2 | |
| 1.27 | 2.63 | 0.65 | 1.35 | 17.51 | 21.04 | 2.66 | 350.07 | 0.2576 | 777.4 | 709.0 | |
| 5.72 | 6.36 | 2.93 | 3.25 | 17.20 | 20.81 | 2.43 | 350.70 | 0.2517 | 1047.7 | 826.4 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 17.83 | 20.66 | 2.28 | 351.65 | 0.2619 | 675.0 | 555.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 17.45 | 20.43 | 2.05 | 352.27 | 0.2550 | 901.0 | 759.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 18.18 | 20.38 | 1.99 | 352.86 | 0.2670 | 767.0 | 634.7 | |
| 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. | |