SDO HMI 2014-08-22 08:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.80 | 50.02 | 10.07 | 26.88 | -9.69 | 333.17 | -15.35 | 137.32 | 0.3871 | 741.8 | 428.4 | |
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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 | 1.98 | 0.00 | 1.04 | -10.18 | 339.18 | -9.35 | 151.37 | 0.3350 | 824.0 | 581.6 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -12.68 | 338.90 | -9.62 | 153.98 | 0.3734 | 757.0 | 628.1 | |
| 0.00 | 1.80 | 0.00 | 0.95 | -10.26 | 338.20 | -10.32 | 149.04 | 0.3441 | 790.0 | 636.3 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -8.62 | 334.55 | -13.97 | 137.95 | 0.3579 | 797.0 | 659.6 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -6.96 | 334.49 | -14.04 | 134.50 | 0.3390 | 708.0 | 578.9 | |
| 0.00 | 0.90 | 0.00 | 0.49 | -11.99 | 334.11 | -14.42 | 142.80 | 0.4044 | -794.0 | -684.2 | |
| 0.00 | 1.80 | 0.00 | 0.94 | -5.42 | 333.90 | -14.62 | 129.90 | 0.3290 | 1008.0 | 792.4 | |
| 18.80 | 31.12 | 10.07 | 16.67 | -9.50 | 333.34 | -15.18 | 137.20 | 0.3818 | 1081.8 | 519.4 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -5.63 | 331.17 | -17.35 | 125.56 | 0.3664 | 709.0 | 598.4 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -5.37 | 330.76 | -17.76 | 124.33 | 0.3694 | 887.0 | 787.4 | |
| 0.00 | 1.26 | 0.00 | 0.68 | -7.04 | 330.02 | -18.50 | 126.79 | 0.3948 | 917.0 | 764.0 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -10.82 | 329.39 | -19.13 | 132.84 | 0.4408 | 675.0 | 507.8 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -14.30 | 327.72 | -20.81 | 135.85 | 0.4962 | -608.0 | -438.5 | |
| 0.00 | 2.61 | 0.00 | 1.50 | -15.42 | 327.47 | -21.06 | 137.09 | 0.5108 | -452.0 | -301.0 | |
| 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. | |