SDO HMI 2011-11-19 11:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 29.27 | 0.00 | 15.09 | 16.90 | 312.00 | -5.80 | 2.34 | 0.2771 | -739.4 | -638.7 | |
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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 | 1.29 | 0.00 | 0.64 | 10.50 | 319.83 | 2.03 | 346.20 | 0.1466 | -712.0 | -521.7 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 17.98 | 316.82 | -0.99 | 3.48 | 0.2711 | -876.0 | -719.3 | |
| 0.00 | 4.38 | 0.00 | 2.25 | 17.89 | 316.57 | -1.24 | 4.38 | 0.2698 | -826.0 | -706.8 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 17.68 | 316.51 | -1.30 | 4.66 | 0.2663 | -1002.0 | -790.0 | |
| 0.00 | 1.46 | 0.00 | 0.74 | 13.14 | 316.30 | -1.51 | 7.81 | 0.1898 | -781.0 | -713.6 | |
| 0.00 | 1.29 | 0.00 | 0.66 | 16.50 | 311.75 | -6.06 | 22.47 | 0.2658 | -1002.0 | -831.9 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 16.25 | 311.48 | -6.33 | 23.75 | 0.2638 | -1080.0 | -945.9 | |
| 0.00 | 3.43 | 0.00 | 1.77 | 16.83 | 311.43 | -6.38 | 23.02 | 0.2731 | -925.0 | -701.5 | |
| 0.00 | 4.55 | 0.00 | 2.34 | 17.11 | 311.30 | -6.51 | 23.04 | 0.2782 | -832.0 | -714.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | 14.15 | 310.07 | -7.74 | 32.53 | 0.2440 | -844.0 | -619.2 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 18.23 | 308.52 | -9.29 | 29.23 | 0.3154 | -719.0 | -534.0 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 14.28 | 306.87 | -10.94 | 41.56 | 0.2784 | 890.0 | 706.1 | |
| 0.00 | 3.43 | 0.00 | 1.81 | 19.17 | 306.13 | -11.67 | 33.38 | 0.3489 | -923.0 | -699.7 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 19.29 | 305.87 | -11.94 | 33.76 | 0.3529 | -719.0 | -549.4 | |
| 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. | |