SDO HMI 2011-10-12 09:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.44 | 32.66 | 3.84 | 17.02 | 21.24 | 109.74 | 9.74 | 329.03 | 0.3090 | 540.0 | 506.8 | |
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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 | 0.70 | 0.00 | 0.37 | 22.47 | 113.37 | 13.38 | 323.10 | 0.3578 | 815.0 | 678.8 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 22.32 | 113.19 | 13.20 | 323.19 | 0.3541 | 852.0 | 606.8 | |
| 0.00 | 2.10 | 0.00 | 1.13 | 24.83 | 113.22 | 13.22 | 327.35 | 0.3865 | 759.0 | 611.0 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 25.75 | 113.32 | 13.33 | 328.53 | 0.3994 | 776.0 | 616.8 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 24.58 | 112.92 | 12.93 | 327.55 | 0.3807 | 718.0 | 543.5 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 20.04 | 112.24 | 12.24 | 320.72 | 0.3161 | -922.0 | -757.2 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 20.42 | 111.94 | 11.95 | 322.17 | 0.3177 | -837.0 | -626.8 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 20.09 | 111.49 | 11.50 | 322.52 | 0.3090 | -979.0 | -714.8 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 26.23 | 111.60 | 11.60 | 332.49 | 0.3923 | 845.0 | 581.8 | |
| 0.00 | 0.53 | 0.00 | 0.28 | 26.36 | 111.41 | 11.41 | 333.04 | 0.3928 | 591.0 | 677.7 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 26.52 | 111.32 | 11.33 | 333.42 | 0.3944 | 684.0 | 517.3 | |
| 3.59 | 19.52 | 1.85 | 10.04 | 19.25 | 108.44 | 8.44 | 328.80 | 0.2689 | 1052.2 | 795.0 | |
| 3.41 | -12.00 | 1.76 | -12.00 | 19.56 | 108.36 | 8.36 | 329.66 | 0.2726 | 1062.6 | 999999 | |
| 0.44 | -12.00 | 0.23 | -12.00 | 19.59 | 108.14 | 8.14 | 330.38 | 0.2712 | 973.4 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 27.62 | 103.90 | 3.90 | 350.67 | 0.3739 | 778.0 | 617.4 | |
| 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. | |