SDO HMI 2011-06-25 00:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.72 | 44.48 | 10.21 | 46.39 | 16.97 | 166.32 | 60.83 | 288.18 | 0.8808 | -132.0 | -110.1 | |
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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 | 0.82 | 0.00 | 0.89 | 15.95 | 167.87 | 62.37 | 286.85 | 0.8919 | -408.0 | -385.9 | |
| 3.72 | 8.08 | 4.04 | 8.76 | 16.56 | 167.72 | 62.23 | 287.54 | 0.8914 | -581.8 | -552.5 | |
| 0.00 | 1.18 | 0.00 | 1.40 | 19.98 | 169.99 | 64.50 | 291.04 | 0.9106 | 383.0 | 322.1 | |
| 0.00 | 1.54 | 0.00 | 1.64 | 16.10 | 167.20 | 61.70 | 287.09 | 0.8869 | -608.0 | -535.9 | |
| 0.00 | 0.54 | 0.00 | 0.57 | 16.43 | 166.70 | 61.21 | 287.52 | 0.8834 | -360.0 | -364.2 | |
| 1.82 | 5.90 | 1.86 | 6.07 | 16.01 | 166.02 | 60.53 | 287.13 | 0.8776 | 260.4 | -82.1 | |
| 1.00 | 2.00 | 1.09 | 2.17 | 19.25 | 167.58 | 62.09 | 290.56 | 0.8929 | -392.8 | -266.3 | |
| 0.00 | 1.18 | 0.00 | 1.21 | 16.71 | 165.87 | 60.38 | 287.95 | 0.8771 | 29.0 | -62.8 | |
| 0.00 | 1.45 | 0.00 | 1.50 | 17.70 | 166.02 | 60.53 | 289.04 | 0.8793 | 117.0 | 72.6 | |
| 2.09 | 20.43 | 2.12 | 20.86 | 16.88 | 165.51 | 60.01 | 288.19 | 0.8744 | 332.7 | 32.5 | |
| 1.09 | -10.00 | 1.10 | -10.00 | 17.11 | 165.50 | 60.01 | 288.44 | 0.8745 | 512.7 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.32 | 18.79 | 163.71 | 58.22 | 290.65 | 0.8620 | -399.0 | -276.7 | |
| 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. | |