SDO HMI 2014-08-13 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 71.09 | 392.43 | 38.77 | 213.79 | 15.07 | 133.70 | 23.49 | 292.21 | 0.4174 | -929.8 | -358.4 | |
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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 | 1.53 | 0.00 | 0.85 | 16.85 | 135.40 | 25.18 | 294.92 | 0.4509 | 683.0 | 523.2 | |
| 0.00 | 1.44 | 0.00 | 0.80 | 16.05 | 135.22 | 25.00 | 293.36 | 0.4443 | -661.0 | -540.8 | |
| 69.56 | 370.53 | 37.99 | 202.29 | 15.18 | 134.03 | 23.82 | 292.26 | 0.4229 | -1342.3 | -408.5 | |
| 0.00 | 1.53 | 0.00 | 0.83 | 16.32 | 131.94 | 21.73 | 296.56 | 0.3988 | -863.0 | -665.1 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 16.51 | 131.80 | 21.58 | 297.14 | 0.3979 | -925.0 | -804.6 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 12.81 | 127.38 | 17.17 | 291.61 | 0.3109 | 813.0 | 622.9 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 12.53 | 127.30 | 17.08 | 290.86 | 0.3082 | 727.0 | 577.0 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 12.48 | 127.00 | 16.79 | 290.99 | 0.3033 | 936.0 | 847.7 | |
| 0.00 | 2.53 | 0.00 | 1.31 | 12.22 | 126.76 | 16.54 | 290.39 | 0.2982 | 720.0 | 681.9 | |
| 0.00 | 1.26 | 0.00 | 0.67 | 19.59 | 126.83 | 16.62 | 310.51 | 0.3559 | 703.0 | 531.6 | |
| 0.00 | 2.98 | 0.00 | 1.53 | 10.40 | 125.52 | 15.31 | 285.32 | 0.2704 | 763.0 | 689.3 | |
| 0.00 | 1.80 | 0.00 | 0.93 | 10.84 | 125.03 | 14.82 | 287.37 | 0.2643 | 951.0 | 793.5 | |
| 1.53 | 4.24 | 0.78 | 2.17 | 10.28 | 124.21 | 13.99 | 286.06 | 0.2487 | 1113.9 | 831.1 | |
| 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. | |