SDO HMI 2011-06-14 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 |
| 49.58 | 269.76 | 140.66 | 809.01 | 16.21 | 165.66 | -79.96 | 73.67 | 0.9841 | -74.4 | -7.9 | |
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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 |
| 9.79 | 140.59 | 18.84 | 278.07 | 16.78 | 170.91 | -74.70 | 72.87 | 0.9675 | -546.4 | -62.1 | |
| 5.53 | -1.00 | 10.94 | -1.00 | 16.87 | 170.56 | -75.05 | 72.80 | 0.9690 | 270.2 | 999999 | |
| 5.71 | -1.00 | 11.34 | -1.00 | 16.13 | 170.39 | -75.23 | 73.57 | 0.9695 | -406.1 | 999999 | |
| 5.35 | -1.00 | 10.86 | -1.00 | 16.25 | 170.12 | -75.49 | 73.46 | 0.9706 | 338.0 | 999999 | |
| 0.00 | 1.18 | 0.00 | 2.92 | 17.43 | 167.43 | -78.18 | 72.39 | 0.9807 | 374.0 | 373.2 | |
| 0.00 | 5.80 | 0.00 | 14.32 | 17.11 | 167.44 | -78.18 | 72.72 | 0.9806 | 172.0 | 172.1 | |
| 2.45 | 24.93 | 10.14 | 106.90 | 18.06 | 162.52 | -83.10 | 71.92 | 0.9934 | 188.4 | 21.4 | |
| 0.00 | 19.94 | 0.00 | 78.61 | 17.30 | 162.93 | -82.69 | 72.68 | 0.9926 | 534.0 | 346.0 | |
| 0.00 | 1.36 | 0.00 | 6.08 | 17.64 | 162.01 | -83.61 | 72.35 | 0.9943 | 309.0 | 185.9 | |
| 2.08 | 17.95 | 9.04 | 87.05 | 16.78 | 162.37 | -83.24 | 73.21 | 0.9936 | 299.3 | -150.0 | |
| 0.00 | 1.90 | 0.00 | 6.54 | 15.47 | 164.06 | -81.55 | 74.50 | 0.9900 | 327.0 | 335.4 | |
| 1.36 | -10.00 | 6.09 | -10.00 | 16.30 | 161.93 | -83.68 | 73.70 | 0.9944 | -204.6 | 999999 | |
| 2.81 | 56.11 | 9.05 | 228.52 | 15.00 | 164.49 | -81.12 | 74.96 | 0.9889 | -225.5 | -100.5 | |
| 9.70 | -13.00 | 34.69 | -13.00 | 14.26 | 163.62 | -82.00 | 75.73 | 0.9909 | -193.8 | 999999 | |
| 4.80 | -13.00 | 19.67 | -13.00 | 14.15 | 162.58 | -83.03 | 75.85 | 0.9931 | 56.7 | 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. | |