SDO HMI 2011-11-27 21:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.45 | 32.41 | 0.76 | 16.94 | 18.15 | 214.77 | 7.92 | 335.77 | 0.3210 | 218.4 | 373.3 | |
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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 | 1.37 | 0.00 | 0.72 | 17.05 | 218.86 | 12.01 | 323.75 | 0.3379 | 671.0 | 657.1 | |
| 0.00 | 1.37 | 0.00 | 0.72 | 18.26 | 218.24 | 11.39 | 327.23 | 0.3481 | 800.0 | 670.8 | |
| 0.00 | 4.02 | 0.00 | 2.10 | 16.29 | 217.80 | 10.95 | 324.78 | 0.3177 | -1069.0 | -888.5 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 17.61 | 217.63 | 10.78 | 327.57 | 0.3339 | 928.0 | 736.3 | |
| 0.00 | 1.97 | 0.00 | 1.05 | 21.01 | 216.28 | 9.43 | 335.57 | 0.3715 | 690.0 | 552.5 | |
| 0.00 | 2.39 | 0.00 | 1.27 | 20.38 | 216.11 | 9.26 | 335.19 | 0.3613 | 809.0 | 655.4 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.16 | 215.69 | 8.84 | 331.72 | 0.3112 | -817.0 | -678.8 | |
| 0.00 | 1.11 | 0.00 | 0.58 | 17.65 | 215.71 | 8.86 | 332.43 | 0.3185 | -710.0 | -650.6 | |
| 0.00 | 0.94 | 0.00 | 0.49 | 15.63 | 214.96 | 8.11 | 331.17 | 0.2832 | -892.0 | -632.7 | |
| 1.45 | 13.17 | 0.76 | 6.84 | 17.91 | 212.93 | 6.08 | 340.53 | 0.3038 | 922.7 | 805.4 | |
| 0.00 | 1.20 | 0.00 | 0.62 | 18.00 | 212.69 | 5.84 | 341.36 | 0.3040 | 810.0 | 688.3 | |
| 0.00 | 2.82 | 0.00 | 1.48 | 20.05 | 212.16 | 5.31 | 344.84 | 0.3338 | 647.0 | 621.3 | |
| 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. | |