SDO HMI 2014-04-11 21:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.47 | 0.00 | 11.41 | -20.91 | 322.37 | 21.94 | 230.66 | 0.4533 | 34.6 | -105.0 | |
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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 | 0.62 | 0.00 | 0.36 | -14.03 | 332.61 | 32.18 | 253.08 | 0.5422 | 504.0 | 398.3 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -17.25 | 332.66 | 32.23 | 247.38 | 0.5539 | 697.0 | 556.6 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -17.18 | 331.02 | 30.59 | 246.68 | 0.5315 | 769.0 | 700.1 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -18.85 | 330.90 | 30.47 | 243.63 | 0.5377 | 487.0 | 442.6 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -18.52 | 330.65 | 30.22 | 244.06 | 0.5328 | 732.0 | 569.6 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -15.74 | 328.41 | 27.98 | 247.96 | 0.4891 | 613.0 | 459.4 | |
| 0.00 | 1.15 | 0.00 | 0.65 | -18.23 | 327.53 | 27.10 | 242.55 | 0.4895 | 700.0 | 577.4 | |
| 0.00 | 1.50 | 0.00 | 0.84 | -18.79 | 325.32 | 24.89 | 239.74 | 0.4633 | 740.0 | 618.9 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -23.66 | 317.02 | 16.59 | 220.21 | 0.4068 | -905.0 | -713.1 | |
| 0.00 | 0.62 | 0.00 | 0.33 | -21.83 | 315.96 | 15.52 | 221.74 | 0.3748 | -692.0 | -626.0 | |
| 0.00 | 1.68 | 0.00 | 0.90 | -21.99 | 315.94 | 15.51 | 221.42 | 0.3764 | -884.0 | -751.2 | |
| 0.00 | 5.12 | 0.00 | 2.77 | -24.23 | 316.03 | 15.60 | 217.62 | 0.4035 | -563.0 | -683.3 | |
| 0.00 | 1.50 | 0.00 | 0.81 | -25.00 | 314.35 | 13.92 | 213.42 | 0.3974 | -893.0 | -768.6 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -24.52 | 314.16 | 13.73 | 213.81 | 0.3897 | -820.0 | -610.7 | |
| 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. | |