SDO HMI 2011-06-04 05:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.52 | 144.83 | 12.43 | 76.74 | -21.00 | 18.75 | -1.96 | 175.02 | 0.3570 | 716.2 | 482.7 | |
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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 | 0.81 | 0.00 | 0.43 | -21.32 | 20.93 | 0.22 | 180.57 | 0.3600 | -884.0 | -603.9 | |
| 23.52 | 115.96 | 12.43 | 61.28 | -20.70 | 19.30 | -1.41 | 176.22 | 0.3506 | 1353.1 | 511.5 | |
| 0.00 | 1.90 | 0.00 | 1.01 | -20.99 | 18.55 | -2.16 | 174.31 | 0.3564 | 937.0 | 691.8 | |
| 0.00 | 1.72 | 0.00 | 0.91 | -21.29 | 18.48 | -2.23 | 174.21 | 0.3612 | 1004.0 | 788.2 | |
| 0.00 | 1.63 | 0.00 | 0.87 | -22.43 | 18.39 | -2.31 | 174.34 | 0.3799 | 703.0 | 553.3 | |
| 0.00 | 5.79 | 0.00 | 3.09 | -21.78 | 18.08 | -2.63 | 173.35 | 0.3699 | 627.0 | 776.4 | |
| 0.00 | 2.44 | 0.00 | 1.30 | -21.52 | 18.08 | -2.63 | 173.28 | 0.3656 | 910.0 | 772.9 | |
| 0.00 | 1.36 | 0.00 | 0.72 | -22.04 | 17.61 | -3.10 | 172.30 | 0.3750 | 872.0 | 754.5 | |
| 0.00 | 5.52 | 0.00 | 2.94 | -21.84 | 17.48 | -3.22 | 171.91 | 0.3722 | 829.0 | 726.8 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -22.27 | 17.47 | -3.23 | 172.05 | 0.3790 | 795.0 | 521.1 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -22.50 | 12.60 | -8.10 | 160.97 | 0.4010 | -844.0 | -682.2 | |
| 0.00 | 1.81 | 0.00 | 0.98 | -23.35 | 12.18 | -8.52 | 160.83 | 0.4161 | -793.0 | -651.2 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -24.25 | 11.42 | -9.29 | 160.06 | 0.4334 | -736.0 | -617.9 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -21.68 | 11.10 | -9.61 | 156.93 | 0.3976 | -581.0 | -526.5 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -26.33 | 9.29 | -11.42 | 157.97 | 0.4751 | -730.0 | -624.1 | |
| 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. | |