SDO HMI 2011-11-19 00:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.26 | 0.00 | 8.99 | 16.86 | 313.78 | -10.04 | 32.97 | 0.3080 | -676.6 | -566.3 | |
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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 | 0.86 | 0.00 | 0.44 | 17.81 | 318.72 | -5.10 | 17.70 | 0.2797 | -742.0 | -595.4 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.29 | 317.51 | -6.31 | 20.87 | 0.2941 | -782.0 | -616.6 | |
| 0.00 | 2.57 | 0.00 | 1.33 | 17.92 | 317.40 | -6.42 | 21.70 | 0.2891 | -1000.0 | -860.5 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 17.89 | 317.06 | -6.76 | 22.78 | 0.2907 | -824.0 | -679.6 | |
| 0.00 | 1.72 | 0.00 | 0.89 | 17.86 | 316.56 | -7.26 | 24.32 | 0.2936 | -734.0 | -608.4 | |
| 0.00 | 1.29 | 0.00 | 0.67 | 17.46 | 316.26 | -7.56 | 25.80 | 0.2897 | -835.0 | -602.1 | |
| 0.00 | 1.03 | 0.00 | 0.52 | 13.35 | 315.92 | -7.90 | 35.17 | 0.2333 | -845.0 | -589.0 | |
| 0.00 | 0.69 | 0.00 | 0.36 | 16.74 | 314.67 | -9.16 | 31.60 | 0.2922 | -766.0 | -618.8 | |
| 0.00 | 0.77 | 0.00 | 0.40 | 17.66 | 313.48 | -10.34 | 33.01 | 0.3153 | -726.0 | -608.4 | |
| 0.00 | 1.37 | 0.00 | 0.71 | 11.87 | 311.01 | -12.81 | 52.75 | 0.2739 | -904.0 | -766.0 | |
| 0.00 | 0.69 | 0.00 | 0.36 | 14.03 | 310.36 | -13.46 | 48.15 | 0.3045 | -695.0 | -561.4 | |
| 0.00 | 1.72 | 0.00 | 0.91 | 18.11 | 309.69 | -14.13 | 40.51 | 0.3587 | -810.0 | -660.0 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 18.30 | 309.42 | -14.40 | 40.69 | 0.3638 | -662.0 | -505.2 | |
| 0.00 | 0.34 | 0.00 | 0.19 | 19.28 | 306.13 | -17.69 | 44.52 | 0.4109 | -433.0 | -245.8 | |
| 0.00 | 1.29 | 0.00 | 0.69 | 15.92 | 305.30 | -18.52 | 52.39 | 0.3873 | 609.0 | 493.3 | |
| 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. | |