SDO HMI 2014-09-22 23:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.18 | 0.00 | 8.81 | -15.16 | 285.80 | -5.05 | 168.24 | 0.4013 | 706.6 | 596.0 | |
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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 | 1.59 | 0.00 | 0.84 | -10.18 | 299.98 | 9.13 | 207.93 | 0.3349 | 670.0 | 633.8 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -10.66 | 298.70 | 7.84 | 203.88 | 0.3328 | 621.0 | 508.0 | |
| 0.00 | 0.80 | 0.00 | 0.42 | -12.05 | 298.64 | 7.79 | 202.12 | 0.3536 | 675.0 | 587.7 | |
| 0.00 | 1.59 | 0.00 | 0.85 | -14.65 | 287.66 | -3.19 | 171.70 | 0.3750 | 676.0 | 389.2 | |
| 0.00 | 1.50 | 0.00 | 0.87 | -23.82 | 284.86 | -6.00 | 169.43 | 0.5233 | 489.0 | 578.1 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -7.99 | 283.84 | -7.01 | 154.94 | 0.2867 | 793.0 | 664.8 | |
| 0.00 | 1.06 | 0.00 | 0.55 | -8.18 | 283.71 | -7.14 | 154.82 | 0.2905 | 744.0 | 667.7 | |
| 0.00 | 1.06 | 0.00 | 0.59 | -19.32 | 282.80 | -8.05 | 163.38 | 0.4642 | 616.0 | 414.4 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -22.29 | 282.44 | -8.42 | 164.51 | 0.5092 | 688.0 | 511.3 | |
| 0.00 | 3.10 | 0.00 | 1.64 | -11.63 | 282.33 | -8.52 | 155.53 | 0.3520 | 778.0 | 682.5 | |
| 0.00 | 1.77 | 0.00 | 0.93 | -10.56 | 282.02 | -8.83 | 153.38 | 0.3383 | 1040.0 | 850.2 | |
| 0.00 | 1.68 | 0.00 | 1.00 | -24.54 | 280.00 | -10.85 | 161.83 | 0.5513 | 689.0 | 488.1 | |
| 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. | |