| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 11.36 | 0.00 | 7.02 | -21.98 | 169.51 | -31.35 | 123.27 | 0.5964 | -279.5 | -227.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-04-19 10:00:34 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 | 1.42 | 0.00 | 0.81 | -32.62 | 186.99 | -13.87 | 156.39 | 0.5061 | 773.0 | 644.0 | |
| 0.00 | 1.15 | 0.00 | 0.69 | -36.90 | 185.80 | -15.06 | 158.48 | 0.5688 | 556.0 | 440.5 | |
| 0.00 | 1.06 | 0.00 | 0.67 | -27.16 | 168.24 | -32.61 | 128.83 | 0.6178 | -731.0 | -520.3 | |
| 0.00 | 1.33 | 0.00 | 0.79 | -19.25 | 170.20 | -30.66 | 117.81 | 0.5464 | -717.0 | -522.3 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -14.36 | 169.92 | -30.94 | 108.93 | 0.5286 | -682.0 | -529.9 | |
| 0.00 | 0.80 | 0.00 | 0.48 | -18.28 | 167.52 | -33.34 | 114.67 | 0.5765 | -553.0 | -520.0 | |
| 0.00 | 1.60 | 0.00 | 1.04 | -18.94 | 161.82 | -39.03 | 113.25 | 0.6506 | -637.0 | -519.7 | |
| 0.00 | 0.98 | 0.00 | 0.62 | -11.56 | 162.57 | -38.29 | 102.02 | 0.6229 | -75.0 | -124.2 | |
| 0.00 | 1.15 | 0.00 | 0.76 | -18.59 | 160.64 | -40.22 | 112.32 | 0.6639 | -212.0 | -303.6 | |
| 0.00 | 0.89 | 0.00 | 0.59 | -18.77 | 160.46 | -40.40 | 112.52 | 0.6665 | -517.0 | -459.0 | |
| 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. | |