| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.67 | 40.49 | 4.49 | 31.88 | -18.11 | 217.65 | 49.50 | 248.36 | 0.7797 | -111.2 | -105.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-05-19 03:00:38 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 |
| 0.00 | 0.54 | 0.00 | 0.45 | -20.00 | 220.18 | 52.03 | 246.67 | 0.8089 | -418.0 | -343.7 | |
| 0.99 | 2.34 | 0.79 | 1.86 | -17.89 | 218.25 | 50.10 | 248.79 | 0.7854 | 671.7 | 549.7 | |
| 3.15 | 20.06 | 2.52 | 16.06 | -18.36 | 218.39 | 50.24 | 248.23 | 0.7878 | 654.7 | 137.8 | |
| 0.00 | 0.81 | 0.00 | 0.64 | -17.49 | 217.90 | 49.75 | 249.21 | 0.7809 | 507.0 | 429.9 | |
| 0.00 | 1.71 | 0.00 | 1.35 | -18.90 | 217.45 | 49.30 | 247.32 | 0.7797 | -610.0 | -481.5 | |
| 0.00 | 0.90 | 0.00 | 0.71 | -18.71 | 217.33 | 49.18 | 247.52 | 0.7780 | -430.0 | -329.4 | |
| 0.99 | 6.66 | 0.77 | 5.17 | -18.56 | 216.98 | 48.83 | 247.62 | 0.7740 | -545.3 | -571.6 | |
| 0.00 | 2.16 | 0.00 | 1.63 | -15.93 | 216.06 | 47.91 | 250.74 | 0.7582 | -606.0 | -466.3 | |
| 0.54 | 1.71 | 0.41 | 1.30 | -16.59 | 216.08 | 47.93 | 249.89 | 0.7599 | -306.5 | -296.8 | |
| 0.00 | 1.35 | 0.00 | 1.02 | -17.01 | 215.66 | 47.51 | 249.23 | 0.7563 | -419.0 | -350.1 | |
| 0.00 | 1.17 | 0.00 | 0.88 | -17.26 | 215.69 | 47.54 | 248.92 | 0.7574 | -472.0 | -300.0 | |
| 0.00 | 1.08 | 0.00 | 0.81 | -17.43 | 215.33 | 47.18 | 248.60 | 0.7539 | -380.0 | -511.8 | |
| 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. | |