SDO HMI 2011-06-07 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.15 | 139.91 | 12.64 | 70.36 | 9.65 | 336.56 | -0.05 | 356.99 | 0.1689 | -688.3 | -436.9 | |
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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 | 0.82 | 7.94 | 339.46 | 2.84 | 340.24 | 0.1460 | -981.0 | -811.4 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 8.34 | 339.34 | 2.72 | 341.89 | 0.1519 | -857.0 | -715.9 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 11.24 | 337.96 | 1.35 | 353.19 | 0.1959 | -771.0 | -506.0 | |
| 22.89 | 120.89 | 11.50 | 60.74 | 9.54 | 336.97 | 0.36 | 357.86 | 0.1653 | -1425.2 | -473.8 | |
| 2.26 | -4.00 | 1.14 | -4.00 | 9.29 | 336.63 | 0.02 | 359.89 | 0.1609 | -975.4 | 999999 | |
| 0.00 | 3.26 | 0.00 | 1.63 | 7.97 | 336.54 | -0.07 | 0.54 | 0.1380 | -1211.0 | -945.4 | |
| 0.00 | 2.17 | 0.00 | 1.09 | 8.74 | 336.23 | -0.38 | 2.51 | 0.1514 | -1161.0 | -960.0 | |
| 0.00 | 1.99 | 0.00 | 1.00 | 8.21 | 335.52 | -1.09 | 7.57 | 0.1435 | -1005.0 | -835.2 | |
| 0.00 | 1.63 | 0.00 | 0.83 | 12.05 | 330.90 | -5.71 | 25.15 | 0.2301 | 802.0 | 591.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 16.03 | 330.39 | -6.23 | 20.78 | 0.2952 | 816.0 | 649.9 | |
| 0.00 | 1.00 | 0.00 | 0.50 | 7.02 | 329.75 | -6.86 | 44.45 | 0.1701 | 971.0 | 884.6 | |
| 0.00 | 0.81 | 0.00 | 0.42 | 14.73 | 329.54 | -7.08 | 25.21 | 0.2809 | 901.0 | 633.1 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 14.80 | 329.19 | -7.43 | 26.19 | 0.2844 | 769.0 | 576.2 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 13.29 | 329.20 | -7.41 | 28.76 | 0.2620 | 738.0 | 564.3 | |
| 0.00 | 0.72 | 0.00 | 0.38 | 17.52 | 326.18 | -10.44 | 29.95 | 0.3475 | 842.0 | 613.0 | |
| 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. | |