SDO HMI 2014-04-09 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.29 | 0.00 | 8.62 | -14.14 | 300.08 | -33.91 | 106.36 | 0.5666 | -160.8 | -118.0 | |
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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 | 1.15 | 0.00 | 0.64 | -5.38 | 305.95 | -28.03 | 90.10 | 0.4698 | 745.0 | 587.2 | |
| 0.00 | 1.85 | 0.00 | 1.01 | -11.15 | 309.39 | -24.60 | 103.56 | 0.4219 | 835.0 | 701.2 | |
| 0.00 | 0.62 | 0.00 | 0.35 | -19.99 | 308.77 | -25.22 | 122.04 | 0.4742 | 797.0 | 696.6 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -20.56 | 305.54 | -28.44 | 120.50 | 0.5196 | 756.0 | 636.7 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -13.93 | 299.58 | -34.41 | 105.80 | 0.5722 | -567.0 | -455.7 | |
| 0.00 | 0.79 | 0.00 | 0.48 | -15.61 | 300.09 | -33.90 | 108.87 | 0.5698 | -697.0 | -592.2 | |
| 0.00 | 0.62 | 0.00 | 0.38 | -15.19 | 297.91 | -36.08 | 107.44 | 0.5979 | -614.0 | -497.3 | |
| 0.00 | 1.50 | 0.00 | 0.95 | -12.06 | 295.57 | -38.41 | 101.82 | 0.6231 | -598.0 | -530.2 | |
| 0.00 | 0.97 | 0.00 | 0.62 | -12.39 | 295.16 | -38.82 | 102.29 | 0.6289 | -432.0 | -409.5 | |
| 0.00 | 1.59 | 0.00 | 1.00 | -13.98 | 295.78 | -38.21 | 104.93 | 0.6235 | -723.0 | -458.6 | |
| 0.00 | 1.50 | 0.00 | 0.95 | -16.39 | 296.36 | -37.62 | 108.92 | 0.6214 | -523.0 | -469.6 | |
| 0.00 | 0.88 | 0.00 | 0.56 | -16.35 | 296.15 | -37.83 | 108.79 | 0.6240 | -620.0 | -465.5 | |
| 0.00 | 0.62 | 0.00 | 0.39 | -16.34 | 295.92 | -38.06 | 108.71 | 0.6269 | -450.0 | -365.0 | |
| 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. | |