SDO HMI 2011-06-03 09:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.21 | 38.89 | 6.01 | 20.49 | 17.06 | 40.50 | 8.74 | 335.33 | 0.3396 | -90.9 | 272.9 | |
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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 |
| 9.13 | 12.48 | 4.91 | 6.71 | 18.06 | 45.53 | 13.78 | 324.43 | 0.3909 | -993.4 | -628.1 | |
| 0.00 | 0.63 | 0.00 | 0.34 | 17.00 | 45.28 | 13.53 | 323.20 | 0.3752 | -772.0 | -575.9 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 16.20 | 42.92 | 11.17 | 326.94 | 0.3426 | -870.0 | -699.5 | |
| 2.08 | 2.62 | 1.10 | 1.38 | 16.96 | 41.55 | 9.80 | 331.41 | 0.3415 | -904.4 | -738.2 | |
| 0.00 | 0.90 | 0.00 | 0.48 | 16.71 | 41.53 | 9.78 | 331.06 | 0.3378 | -997.0 | -798.5 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.33 | 41.06 | 9.31 | 331.66 | 0.3286 | -888.0 | -696.3 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 16.70 | 38.10 | 6.35 | 340.20 | 0.3142 | 907.0 | 715.1 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.80 | 37.43 | 5.68 | 342.24 | 0.3121 | 884.0 | 664.7 | |
| 0.00 | 3.71 | 0.00 | 1.93 | 16.54 | 37.17 | 5.42 | 342.75 | 0.3067 | 729.0 | 594.9 | |
| 0.00 | 2.17 | 0.00 | 1.13 | 16.45 | 36.91 | 5.16 | 343.43 | 0.3040 | 882.0 | 697.1 | |
| 0.00 | 3.62 | 0.00 | 1.88 | 16.22 | 36.21 | 4.46 | 345.39 | 0.2972 | 842.0 | 733.9 | |
| 0.00 | 2.71 | 0.00 | 1.41 | 16.67 | 35.81 | 4.05 | 347.02 | 0.3028 | 779.0 | 746.7 | |
| 0.00 | 2.08 | 0.00 | 1.08 | 16.26 | 35.73 | 3.98 | 346.92 | 0.2958 | 1008.0 | 863.1 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 16.57 | 35.61 | 3.86 | 347.54 | 0.3006 | 829.0 | 657.4 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 17.40 | 35.09 | 3.34 | 349.71 | 0.3124 | 812.0 | 634.0 | |
| 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. | |