| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.25 | 40.76 | 9.36 | 33.60 | -18.24 | 217.64 | 51.69 | 248.72 | 0.8017 | 124.0 | -55.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-05-19 07:00:38 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 |
| 0.54 | 1.62 | 0.45 | 1.36 | -18.06 | 218.43 | 52.47 | 249.12 | 0.8092 | 753.3 | 568.6 | |
| 7.74 | 21.77 | 6.52 | 18.31 | -18.47 | 218.55 | 52.60 | 248.65 | 0.8112 | 659.1 | 157.3 | |
| 0.00 | 0.90 | 0.00 | 0.75 | -17.87 | 218.30 | 52.34 | 249.32 | 0.8076 | 528.0 | 463.8 | |
| 0.00 | 2.97 | 0.00 | 2.45 | -18.81 | 217.50 | 51.54 | 247.98 | 0.8018 | -613.0 | -436.4 | |
| 1.26 | 2.52 | 1.03 | 2.06 | -18.63 | 217.06 | 51.11 | 248.09 | 0.7971 | -612.1 | -458.1 | |
| 0.00 | 1.44 | 0.00 | 1.13 | -15.76 | 215.98 | 50.02 | 251.43 | 0.7803 | -741.0 | -550.9 | |
| 0.72 | 2.70 | 0.58 | 2.18 | -18.46 | 216.53 | 50.58 | 248.18 | 0.7915 | -448.9 | -405.7 | |
| 0.00 | 1.35 | 0.00 | 1.08 | -18.37 | 216.25 | 50.29 | 248.21 | 0.7884 | -529.0 | -357.4 | |
| 0.99 | 2.07 | 0.78 | 1.62 | -17.19 | 215.35 | 49.39 | 249.47 | 0.7767 | -382.1 | -357.8 | |
| 0.00 | 1.17 | 0.00 | 0.92 | -17.44 | 215.39 | 49.43 | 249.16 | 0.7777 | -484.0 | -395.9 | |
| 0.00 | 1.26 | 0.00 | 0.98 | -17.45 | 215.20 | 49.24 | 249.11 | 0.7757 | -722.0 | -528.1 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -17.48 | 214.00 | 48.04 | 248.75 | 0.7633 | 512.0 | 412.0 | |
| 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. | |