SDO HMI 2011-02-12 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 |
| 23.45 | 65.00 | 13.06 | 36.26 | 19.75 | 63.07 | 7.30 | 344.93 | 0.4623 | 660.0 | 436.7 | |
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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 | 1.37 | 0.00 | 0.77 | 19.89 | 65.79 | 10.02 | 339.84 | 0.4768 | -700.0 | -690.5 | |
| 0.00 | 1.63 | 0.00 | 0.91 | 19.76 | 65.75 | 9.98 | 339.82 | 0.4747 | -1041.0 | -863.4 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 19.28 | 65.24 | 9.47 | 340.41 | 0.4652 | -721.0 | -551.8 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 18.96 | 63.89 | 8.12 | 342.80 | 0.4539 | 702.0 | 547.2 | |
| 8.48 | 11.73 | 4.71 | 6.51 | 19.15 | 63.46 | 7.69 | 343.79 | 0.4548 | 1037.6 | 673.8 | |
| 2.05 | 30.65 | 1.14 | 17.09 | 19.51 | 63.22 | 7.45 | 344.49 | 0.4592 | 879.0 | 408.4 | |
| 11.81 | -6.00 | 6.59 | -6.00 | 19.70 | 62.95 | 7.18 | 345.15 | 0.4609 | 961.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 20.60 | 62.76 | 7.00 | 346.01 | 0.4736 | 552.0 | 451.5 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 19.86 | 62.57 | 6.81 | 345.98 | 0.4619 | 873.0 | 730.0 | |
| 1.11 | 11.22 | 0.62 | 6.28 | 20.23 | 62.49 | 6.73 | 346.33 | 0.4671 | 929.4 | 766.6 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 20.59 | 62.35 | 6.58 | 346.80 | 0.4720 | 623.0 | 550.6 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 20.56 | 62.16 | 6.39 | 347.16 | 0.4708 | 813.0 | 650.1 | |
| 0.00 | 1.46 | 0.00 | 0.82 | 20.90 | 60.45 | 4.69 | 350.63 | 0.4710 | 657.0 | 553.1 | |
| 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. | |