SDO HMI 2011-06-14 07:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.61 | 243.34 | 132.10 | 854.37 | 16.29 | 165.66 | -81.59 | 73.63 | 0.9882 | -46.1 | 46.0 | |
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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 |
| 8.61 | 132.46 | 18.44 | 294.56 | 16.72 | 170.92 | -76.33 | 73.02 | 0.9740 | -540.6 | -31.7 | |
| 5.53 | -1.00 | 12.21 | -1.00 | 16.84 | 170.49 | -76.77 | 72.92 | 0.9757 | 314.2 | 999999 | |
| 0.00 | 1.36 | 0.00 | 3.60 | 17.55 | 168.37 | -78.88 | 72.30 | 0.9829 | 324.0 | 297.1 | |
| 5.17 | -1.00 | 11.75 | -1.00 | 16.23 | 170.14 | -77.12 | 73.56 | 0.9768 | 360.1 | 999999 | |
| 4.08 | -1.00 | 9.05 | -1.00 | 16.04 | 170.37 | -76.88 | 73.74 | 0.9759 | -346.5 | 999999 | |
| 0.00 | 11.79 | 0.00 | 33.36 | 17.15 | 167.63 | -79.63 | 72.73 | 0.9851 | -33.0 | 290.3 | |
| 1.90 | 35.72 | 9.99 | 190.23 | 18.04 | 162.62 | -84.64 | 71.96 | 0.9960 | 173.0 | 218.7 | |
| 1.54 | -7.00 | 9.49 | -7.00 | 18.09 | 161.62 | -85.64 | 71.92 | 0.9974 | -232.9 | 999999 | |
| 0.00 | 2.72 | 0.00 | 10.20 | 16.63 | 164.87 | -82.38 | 73.34 | 0.9919 | 53.0 | 148.7 | |
| 0.00 | 4.35 | 0.00 | 31.79 | 16.78 | 161.55 | -85.71 | 73.24 | 0.9974 | -14.0 | -36.7 | |
| 2.63 | 10.61 | 13.27 | 60.35 | 16.22 | 162.79 | -84.47 | 73.79 | 0.9957 | 360.2 | 5.4 | |
| 0.00 | 2.72 | 0.00 | 11.33 | 15.51 | 164.12 | -83.14 | 74.48 | 0.9934 | 354.0 | 332.2 | |
| 7.52 | 41.61 | 33.97 | 218.95 | 14.27 | 163.65 | -83.61 | 75.74 | 0.9942 | -196.6 | -67.2 | |
| 2.63 | -13.00 | 13.93 | -13.00 | 14.19 | 162.56 | -84.70 | 75.83 | 0.9960 | 29.5 | 999999 | |
| 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. | |