SDO HMI 2014-11-16 06:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.89 | 0.00 | 10.40 | -10.68 | 323.37 | 28.63 | 244.39 | 0.5246 | 695.6 | 593.8 | |
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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 | 0.86 | 0.00 | 0.51 | -12.15 | 324.50 | 29.76 | 242.70 | 0.5482 | 466.0 | 378.8 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -11.89 | 324.12 | 29.38 | 242.84 | 0.5417 | 535.0 | 464.7 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -11.43 | 323.86 | 29.12 | 243.43 | 0.5354 | 731.0 | 623.7 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -11.60 | 323.57 | 28.82 | 242.91 | 0.5326 | 744.0 | 624.5 | |
| 0.00 | 1.20 | 0.00 | 0.70 | -11.11 | 323.45 | 28.70 | 243.66 | 0.5279 | 642.0 | 521.9 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -10.10 | 323.31 | 28.56 | 245.33 | 0.5201 | 629.0 | 557.8 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -7.62 | 323.07 | 28.32 | 249.72 | 0.5034 | 823.0 | 703.3 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -11.45 | 323.41 | 28.67 | 243.05 | 0.5296 | 682.0 | 586.0 | |
| 0.00 | 0.69 | 0.00 | 0.40 | -10.89 | 323.32 | 28.57 | 243.94 | 0.5249 | 725.0 | 618.9 | |
| 0.00 | 2.67 | 0.00 | 1.56 | -11.84 | 323.39 | 28.64 | 242.35 | 0.5317 | 563.0 | 545.9 | |
| 0.00 | 4.39 | 0.00 | 2.54 | -10.59 | 323.15 | 28.41 | 244.35 | 0.5208 | 818.0 | 654.1 | |
| 0.00 | 1.38 | 0.00 | 0.79 | -7.73 | 322.84 | 28.09 | 249.35 | 0.5007 | 800.0 | 619.2 | |
| 0.00 | 1.20 | 0.00 | 0.70 | -10.52 | 322.97 | 28.23 | 244.33 | 0.5180 | 885.0 | 681.2 | |
| 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. | |