SDO HMI 2011-07-02 04:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.45 | 20.72 | 0.24 | 10.82 | 16.50 | 23.10 | 12.46 | 318.97 | 0.3168 | 7.7 | 136.7 | |
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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 | 1.73 | 0.00 | 0.93 | 19.96 | 27.36 | 16.72 | 317.43 | 0.4013 | -712.0 | -521.3 | |
| 0.00 | 2.91 | 0.00 | 1.52 | 13.46 | 26.71 | 16.07 | 304.37 | 0.3276 | 971.0 | 861.4 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 16.63 | 25.18 | 14.54 | 314.68 | 0.3398 | -737.0 | -613.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 16.52 | 23.83 | 13.19 | 317.15 | 0.3230 | -738.0 | -553.3 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 16.78 | 23.68 | 13.04 | 318.01 | 0.3244 | -934.0 | -777.3 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 15.75 | 23.06 | 12.42 | 317.06 | 0.3052 | -924.0 | -722.5 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 15.69 | 22.70 | 12.06 | 317.74 | 0.3005 | -785.0 | -604.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 16.67 | 22.14 | 11.50 | 321.23 | 0.3065 | -726.0 | -460.0 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 16.33 | 21.09 | 10.45 | 323.13 | 0.2913 | 1004.0 | 722.1 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 17.43 | 21.05 | 10.41 | 325.47 | 0.3056 | 944.0 | 638.0 | |
| 0.45 | 2.00 | 0.24 | 1.04 | 16.96 | 20.93 | 10.29 | 324.85 | 0.2981 | 975.8 | 779.1 | |
| 0.00 | 2.54 | 0.00 | 1.32 | 16.75 | 20.43 | 9.79 | 325.72 | 0.2904 | 800.0 | 673.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 17.60 | 20.25 | 9.61 | 327.86 | 0.3005 | 729.0 | 647.8 | |
| 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. | |