SDO HMI 2011-06-03 14:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.12 | 29.31 | 6.04 | 15.64 | 17.05 | 41.80 | 12.81 | 325.77 | 0.3722 | -138.8 | 184.9 | |
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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 | 1.63 | 0.00 | 0.88 | 15.84 | 46.88 | 17.88 | 313.41 | 0.4083 | 896.0 | 573.6 | |
| 9.58 | 10.85 | 5.22 | 5.91 | 18.01 | 45.55 | 16.56 | 319.35 | 0.4177 | -986.0 | -696.1 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 18.20 | 44.84 | 15.84 | 320.87 | 0.4126 | -721.0 | -549.2 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 12.60 | 43.79 | 14.79 | 312.05 | 0.3370 | -732.0 | -490.4 | |
| 1.54 | 1.99 | 0.82 | 1.06 | 17.13 | 41.69 | 12.69 | 325.12 | 0.3687 | -805.5 | -817.8 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 16.94 | 41.68 | 12.68 | 324.84 | 0.3661 | -796.0 | -603.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 16.46 | 41.00 | 12.00 | 325.50 | 0.3534 | -971.0 | -765.5 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 16.71 | 38.10 | 9.11 | 332.75 | 0.3324 | 830.0 | 563.8 | |
| 0.00 | 2.08 | 0.00 | 1.09 | 16.71 | 37.37 | 8.37 | 334.66 | 0.3270 | 855.0 | 634.3 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 16.30 | 36.48 | 7.48 | 336.49 | 0.3148 | 885.0 | 733.1 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 16.39 | 36.30 | 7.30 | 337.14 | 0.3150 | 722.0 | 593.1 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 16.78 | 35.86 | 6.86 | 338.82 | 0.3181 | 581.0 | 534.6 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 16.27 | 35.75 | 6.75 | 338.53 | 0.3096 | 1039.0 | 840.0 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.55 | 35.31 | 6.31 | 340.13 | 0.3114 | 715.0 | 613.7 | |
| 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. | |