SDO HMI 2011-07-01 21:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.08 | 34.16 | 5.70 | 17.68 | 16.76 | 23.67 | 9.17 | 327.64 | 0.2887 | -35.0 | -207.6 | |
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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 | 1.54 | 0.00 | 0.82 | 19.95 | 27.29 | 12.79 | 324.72 | 0.3619 | -681.0 | -536.6 | |
| 3.45 | 6.27 | 1.78 | 3.23 | 13.45 | 26.63 | 12.13 | 312.00 | 0.2762 | 1019.5 | 764.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.27 | 25.41 | 10.91 | 319.64 | 0.2832 | -795.0 | -618.3 | |
| 0.00 | 4.09 | 0.00 | 2.17 | 20.96 | 25.71 | 11.21 | 329.70 | 0.3613 | -505.0 | -549.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 16.33 | 25.40 | 10.90 | 322.07 | 0.2966 | -838.0 | -631.7 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 15.71 | 25.30 | 10.80 | 320.93 | 0.2876 | -907.0 | -733.9 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 16.59 | 24.77 | 10.27 | 324.23 | 0.2936 | -882.0 | -624.2 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 16.63 | 23.67 | 9.18 | 327.27 | 0.2838 | -1069.0 | -924.2 | |
| 0.00 | 2.00 | 0.00 | 1.03 | 15.89 | 22.64 | 8.15 | 328.79 | 0.2642 | -1107.0 | -850.5 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.45 | 21.87 | 7.37 | 332.32 | 0.2660 | -814.0 | -604.5 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.84 | 21.28 | 6.78 | 336.46 | 0.2826 | 466.0 | 241.4 | |
| 0.64 | 1.91 | 0.33 | 0.98 | 17.40 | 20.97 | 6.47 | 336.75 | 0.2738 | 921.6 | 676.3 | |
| 3.27 | 5.54 | 1.68 | 2.85 | 17.06 | 20.90 | 6.40 | 336.47 | 0.2680 | 988.6 | 806.8 | |
| 3.72 | 4.09 | 1.91 | 2.10 | 16.62 | 20.56 | 6.06 | 336.89 | 0.2590 | 966.4 | 771.5 | |
| 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. | |