SDO HMI 2011-06-08 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.60 | 29.34 | 9.89 | 27.12 | 17.50 | 20.90 | 55.87 | 290.76 | 0.8458 | -273.9 | -252.8 | |
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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 | 2.17 | 0.00 | 2.25 | 20.16 | 24.43 | 59.40 | 293.01 | 0.8798 | -583.0 | -389.6 | |
| 5.07 | 7.97 | 4.79 | 7.53 | 17.11 | 21.85 | 56.82 | 290.09 | 0.8537 | -416.2 | -315.8 | |
| 0.00 | 1.99 | 0.00 | 1.86 | 17.24 | 21.38 | 56.35 | 290.33 | 0.8500 | -325.0 | -373.9 | |
| 0.00 | 1.18 | 0.00 | 1.09 | 17.11 | 21.21 | 56.18 | 290.22 | 0.8482 | -471.0 | -412.3 | |
| 1.36 | 3.26 | 1.25 | 2.99 | 16.70 | 20.79 | 55.76 | 289.83 | 0.8438 | -523.1 | -414.1 | |
| 0.00 | 1.81 | 0.00 | 1.67 | 16.99 | 20.92 | 55.89 | 290.14 | 0.8455 | -571.0 | -434.2 | |
| 0.00 | 1.54 | 0.00 | 1.40 | 16.32 | 20.57 | 55.54 | 289.43 | 0.8412 | -240.0 | -227.5 | |
| 2.63 | 3.53 | 2.38 | 3.21 | 16.60 | 20.41 | 55.38 | 289.80 | 0.8403 | -687.3 | -634.2 | |
| 1.54 | 1.90 | 1.47 | 1.81 | 19.42 | 21.72 | 56.69 | 292.77 | 0.8568 | 337.5 | 177.0 | |
| 0.00 | 0.91 | 0.00 | 0.83 | 17.62 | 20.76 | 55.73 | 290.92 | 0.8452 | -464.0 | -374.7 | |
| 0.00 | 1.09 | 0.00 | 0.88 | 17.35 | 15.10 | 50.08 | 292.02 | 0.7919 | 443.0 | 504.8 | |
| 0.00 | 0.63 | 0.00 | 0.51 | 17.60 | 15.10 | 50.07 | 292.34 | 0.7925 | 390.0 | 351.0 | |
| 0.00 | 1.36 | 0.00 | 1.09 | 19.43 | 14.23 | 49.20 | 294.85 | 0.7890 | 435.0 | 408.6 | |
| 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. | |