| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.87 | 93.30 | 24.58 | 94.47 | -10.56 | 295.38 | 61.41 | 261.78 | 0.8734 | -200.7 | -147.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-20 15:00:30 UT
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 |
| 2.88 | 8.10 | 3.32 | 9.33 | -9.48 | 299.25 | 65.28 | 262.81 | 0.9049 | 534.8 | 335.5 | |
| 1.39 | 14.98 | 1.60 | 16.96 | -10.08 | 299.26 | 65.29 | 262.14 | 0.9047 | 0.8 | 375.5 | |
| 0.00 | 1.31 | 0.00 | 1.49 | -9.57 | 298.99 | 65.02 | 262.73 | 0.9029 | 458.0 | 416.7 | |
| 2.96 | -2.00 | 3.34 | -2.00 | -9.90 | 298.68 | 64.71 | 262.38 | 0.9005 | 573.0 | 999999 | |
| 1.66 | -2.00 | 1.88 | -2.00 | -10.25 | 298.81 | 64.85 | 261.98 | 0.9013 | 420.6 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.49 | -10.69 | 298.70 | 64.73 | 261.50 | 0.9003 | 315.0 | 308.0 | |
| 0.00 | 1.13 | 0.00 | 1.27 | -10.44 | 298.46 | 64.49 | 261.79 | 0.8986 | 461.0 | 451.3 | |
| 0.00 | 1.05 | 0.00 | 1.04 | -11.56 | 294.80 | 60.83 | 260.67 | 0.8690 | -187.0 | -127.5 | |
| 0.00 | 0.87 | 0.00 | 0.86 | -11.83 | 294.58 | 60.61 | 260.37 | 0.8671 | -294.0 | -251.9 | |
| 0.78 | 2.00 | 0.77 | 1.96 | -11.47 | 294.26 | 60.30 | 260.80 | 0.8644 | -441.3 | -322.6 | |
| 0.96 | 62.55 | 0.93 | 60.22 | -11.03 | 294.05 | 60.08 | 261.31 | 0.8627 | -333.7 | -350.6 | |
| 0.00 | 0.87 | 0.00 | 0.85 | -11.77 | 294.31 | 60.34 | 260.45 | 0.8647 | -591.0 | -479.0 | |
| 9.15 | -11.00 | 8.79 | -11.00 | -10.65 | 293.62 | 59.65 | 261.76 | 0.8590 | -813.8 | 999999 | |
| 4.09 | -11.00 | 3.95 | -11.00 | -11.15 | 293.78 | 59.82 | 261.18 | 0.8603 | -753.7 | 999999 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |