SDO HMI 2011-11-29 15:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.69 | 134.83 | 24.98 | 106.24 | 15.72 | 233.36 | 49.55 | 289.45 | 0.7791 | -744.6 | -236.4 | |
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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 | 1.20 | 0.00 | 0.98 | 16.52 | 235.26 | 51.46 | 289.98 | 0.8002 | -526.0 | -387.5 | |
| 0.00 | 0.77 | 0.00 | 0.64 | 17.84 | 235.58 | 51.78 | 291.52 | 0.8061 | -516.0 | -406.3 | |
| 0.00 | 1.11 | 0.00 | 0.92 | 17.62 | 235.45 | 51.64 | 291.29 | 0.8043 | -584.0 | -495.8 | |
| 1.45 | 2.48 | 1.21 | 2.06 | 18.12 | 235.45 | 51.64 | 291.89 | 0.8054 | -607.0 | -459.3 | |
| 0.00 | 1.54 | 0.00 | 1.28 | 18.40 | 235.46 | 51.66 | 292.23 | 0.8062 | -470.0 | -408.9 | |
| 21.45 | 109.11 | 16.84 | 85.80 | 15.41 | 233.32 | 49.51 | 289.07 | 0.7781 | -911.0 | -189.2 | |
| 1.45 | -6.00 | 1.13 | -6.00 | 15.66 | 233.02 | 49.22 | 289.46 | 0.7756 | -857.0 | 999999 | |
| 0.00 | 1.62 | 0.00 | 1.24 | 13.29 | 232.27 | 48.47 | 286.61 | 0.7626 | -586.0 | -462.5 | |
| 5.55 | 7.86 | 4.39 | 6.21 | 16.91 | 233.31 | 49.50 | 290.96 | 0.7815 | -534.0 | -315.8 | |
| 0.51 | 3.42 | 0.40 | 2.65 | 15.91 | 232.68 | 48.88 | 289.86 | 0.7726 | -763.0 | -669.7 | |
| 1.28 | 2.56 | 1.01 | 2.01 | 16.76 | 232.97 | 49.17 | 290.87 | 0.7776 | -637.3 | -591.2 | |
| 0.00 | 1.11 | 0.00 | 0.84 | 15.25 | 231.55 | 47.74 | 289.32 | 0.7590 | -723.0 | -533.4 | |
| 0.00 | 1.20 | 0.00 | 0.94 | 19.56 | 232.42 | 48.61 | 294.54 | 0.7794 | -453.0 | -393.6 | |
| 0.00 | 0.85 | 0.00 | 0.67 | 19.51 | 231.92 | 48.11 | 294.62 | 0.7742 | -344.0 | -440.1 | |
| 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. | |