SDO HMI 2011-11-22 08:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.26 | 48.51 | 13.20 | 52.17 | -17.08 | 340.38 | 60.48 | 249.55 | 0.8895 | 360.5 | 222.9 | |
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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 | 1.03 | 0.00 | 1.32 | -17.10 | 345.44 | 65.54 | 250.52 | 0.9245 | 348.0 | 246.3 | |
| 1.20 | 4.20 | 1.34 | 4.71 | -16.54 | 341.64 | 61.74 | 250.42 | 0.8981 | -222.0 | -482.1 | |
| 0.43 | 1.71 | 0.48 | 1.91 | -16.75 | 341.63 | 61.73 | 250.18 | 0.8983 | 231.2 | 133.9 | |
| 0.00 | 1.54 | 0.00 | 1.71 | -17.02 | 341.26 | 61.36 | 249.81 | 0.8960 | 258.0 | 199.9 | |
| 0.00 | 0.86 | 0.00 | 0.97 | -17.95 | 341.81 | 61.90 | 248.91 | 0.9013 | -317.0 | -232.0 | |
| 10.63 | 30.52 | 11.38 | 32.61 | -16.68 | 340.30 | 60.40 | 249.98 | 0.8884 | 645.5 | 379.7 | |
| 0.00 | 1.29 | 0.00 | 1.36 | -18.66 | 339.53 | 59.62 | 247.62 | 0.8859 | 151.0 | 104.7 | |
| 0.00 | 1.11 | 0.00 | 1.17 | -18.37 | 339.23 | 59.33 | 247.88 | 0.8832 | 485.0 | 376.8 | |
| 0.00 | 3.00 | 0.00 | 3.14 | -18.65 | 339.15 | 59.24 | 247.54 | 0.8830 | 638.0 | 475.3 | |
| 0.00 | 0.94 | 0.00 | 0.97 | -18.44 | 338.67 | 58.76 | 247.65 | 0.8789 | 341.0 | 436.9 | |
| 0.00 | 1.20 | 0.00 | 1.20 | -19.51 | 337.47 | 57.56 | 246.16 | 0.8717 | -391.0 | -296.4 | |
| 0.00 | 1.11 | 0.00 | 1.10 | -19.31 | 337.00 | 57.10 | 246.27 | 0.8676 | -540.0 | -478.0 | |
| 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. | |