SDO HMI 2014-08-19 22:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.59 | 98.87 | 17.09 | 78.00 | -9.29 | 331.88 | -48.57 | 107.86 | 0.7795 | 714.8 | 338.4 | |
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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 | 1.44 | 0.00 | 1.03 | -10.48 | 337.48 | -42.97 | 111.69 | 0.7235 | 641.0 | 518.8 | |
| 0.00 | 0.63 | 0.00 | 0.45 | -9.22 | 337.56 | -42.88 | 110.06 | 0.7174 | 759.0 | 661.9 | |
| 0.00 | 0.36 | 0.00 | 0.25 | -8.74 | 337.59 | -42.85 | 109.45 | 0.7152 | 698.0 | 644.0 | |
| 0.00 | 1.26 | 0.00 | 0.92 | -9.48 | 335.94 | -44.50 | 109.69 | 0.7366 | 196.0 | 198.3 | |
| 0.00 | 0.63 | 0.00 | 0.46 | -9.18 | 335.77 | -44.67 | 109.23 | 0.7374 | 488.0 | 472.1 | |
| 0.00 | 0.45 | 0.00 | 0.33 | -6.64 | 334.78 | -45.66 | 105.54 | 0.7397 | 535.0 | 501.0 | |
| 16.64 | 75.47 | 13.08 | 59.49 | -9.45 | 332.00 | -48.45 | 108.09 | 0.7788 | 968.8 | 318.3 | |
| 0.00 | 0.36 | 0.00 | 0.29 | -11.85 | 331.00 | -49.45 | 110.62 | 0.7967 | 431.0 | 435.0 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -6.46 | 331.92 | -48.52 | 104.33 | 0.7706 | 633.0 | 547.5 | |
| 0.00 | 1.98 | 0.00 | 1.58 | -9.37 | 331.12 | -49.32 | 107.67 | 0.7876 | 336.0 | 311.2 | |
| 0.00 | 1.44 | 0.00 | 1.18 | -11.48 | 330.56 | -49.88 | 110.01 | 0.7998 | 456.0 | 262.6 | |
| 4.50 | 8.10 | 3.64 | 6.55 | -9.34 | 330.51 | -49.94 | 107.41 | 0.7937 | 657.1 | 482.6 | |
| 0.45 | 1.62 | 0.37 | 1.33 | -9.48 | 329.99 | -50.45 | 107.41 | 0.7993 | 439.6 | 374.5 | |
| 0.00 | 0.99 | 0.00 | 0.80 | -7.15 | 329.84 | -50.61 | 104.52 | 0.7944 | 548.0 | 475.6 | |
| 0.00 | 2.16 | 0.00 | 1.76 | -5.63 | 329.17 | -51.27 | 102.47 | 0.7973 | 374.0 | 291.8 | |
| 0.00 | 1.08 | 0.00 | 0.88 | -5.23 | 329.12 | -51.32 | 101.96 | 0.7969 | 462.0 | 352.2 | |
| 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. | |