SDO HMI 2011-11-22 07:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.83 | 58.31 | 12.50 | 61.51 | -17.10 | 340.34 | 59.89 | 249.38 | 0.8851 | 319.0 | 186.4 | |
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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 | 0.77 | 0.00 | 0.97 | -17.01 | 345.33 | 64.89 | 250.50 | 0.9202 | 292.0 | 273.2 | |
| 0.00 | 0.86 | 0.00 | 1.02 | -16.53 | 344.10 | 63.65 | 250.79 | 0.9115 | 333.0 | 271.0 | |
| 0.00 | 0.77 | 0.00 | 0.86 | -16.44 | 342.00 | 61.56 | 250.49 | 0.8966 | -446.0 | -432.2 | |
| 1.03 | 5.40 | 1.13 | 5.91 | -16.52 | 341.66 | 61.21 | 250.33 | 0.8942 | -300.2 | -428.9 | |
| 0.69 | 3.43 | 0.75 | 3.77 | -16.77 | 341.60 | 61.15 | 250.05 | 0.8941 | 210.8 | -82.4 | |
| 0.00 | 1.11 | 0.00 | 1.24 | -17.96 | 341.77 | 61.32 | 248.77 | 0.8972 | -348.0 | -261.0 | |
| 0.00 | 1.03 | 0.00 | 1.12 | -17.07 | 341.25 | 60.80 | 249.64 | 0.8920 | 344.0 | 271.8 | |
| 9.60 | 33.87 | 10.12 | 35.55 | -16.66 | 340.34 | 59.89 | 249.89 | 0.8845 | 658.2 | 402.0 | |
| 0.00 | 1.89 | 0.00 | 1.97 | -18.64 | 339.57 | 59.12 | 247.52 | 0.8821 | 208.0 | 137.6 | |
| 0.00 | 0.86 | 0.00 | 0.89 | -18.51 | 339.37 | 58.92 | 247.62 | 0.8803 | 447.0 | 376.1 | |
| 0.00 | 0.94 | 0.00 | 0.97 | -18.35 | 339.16 | 58.71 | 247.75 | 0.8784 | 325.0 | 361.8 | |
| 0.00 | 2.14 | 0.00 | 2.21 | -18.73 | 339.19 | 58.74 | 247.33 | 0.8793 | 511.0 | 383.9 | |
| 0.00 | 1.03 | 0.00 | 1.04 | -18.43 | 338.66 | 58.21 | 247.54 | 0.8746 | 517.0 | 425.3 | |
| 0.00 | 1.29 | 0.00 | 1.27 | -19.46 | 337.46 | 57.01 | 246.07 | 0.8673 | -231.0 | -214.0 | |
| 0.51 | 2.06 | 0.50 | 2.00 | -19.26 | 337.00 | 56.55 | 246.17 | 0.8632 | -465.0 | -473.5 | |
| 0.00 | 0.86 | 0.00 | 0.72 | -21.20 | 330.47 | 50.02 | 241.84 | 0.8126 | -384.0 | -282.2 | |
| 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. | |