| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.19 | 39.09 | 11.69 | 32.20 | -23.67 | 95.03 | -48.15 | 121.38 | 0.8011 | -11.1 | 149.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-27 18:00:25 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 | 1.88 | 0.00 | 1.51 | -25.49 | 97.16 | -46.02 | 124.41 | 0.7896 | 51.0 | 140.0 | |
| 3.16 | 12.06 | 2.56 | 9.76 | -24.16 | 96.10 | -47.08 | 122.38 | 0.7934 | 715.0 | 536.4 | |
| 4.19 | 5.90 | 3.35 | 4.72 | -23.31 | 96.41 | -46.77 | 121.51 | 0.7872 | 616.1 | 350.4 | |
| 0.00 | 0.94 | 0.00 | 0.77 | -24.10 | 95.84 | -47.34 | 122.20 | 0.7955 | 433.0 | 345.7 | |
| 0.00 | 1.03 | 0.00 | 0.83 | -23.90 | 95.89 | -47.29 | 121.99 | 0.7943 | 610.0 | 457.2 | |
| 0.00 | 1.97 | 0.00 | 1.59 | -23.71 | 95.84 | -47.34 | 121.74 | 0.7940 | 710.0 | 562.0 | |
| 4.62 | 6.50 | 3.87 | 5.45 | -23.25 | 93.97 | -49.21 | 120.44 | 0.8090 | -737.7 | -534.7 | |
| 0.00 | 0.60 | 0.00 | 0.51 | -23.27 | 93.42 | -49.76 | 120.23 | 0.8139 | -511.0 | -453.0 | |
| 0.00 | 1.54 | 0.00 | 1.31 | -23.07 | 93.31 | -49.86 | 119.97 | 0.8142 | -516.0 | -444.1 | |
| 0.00 | 0.94 | 0.00 | 0.81 | -23.37 | 93.01 | -50.17 | 120.20 | 0.8178 | -182.0 | -247.8 | |
| 0.00 | 0.94 | 0.00 | 0.80 | -22.72 | 93.04 | -50.14 | 119.46 | 0.8154 | -459.0 | -415.8 | |
| 2.22 | 4.11 | 1.91 | 3.53 | -23.08 | 92.70 | -50.47 | 119.75 | 0.8195 | -502.1 | -370.1 | |
| 0.00 | 0.68 | 0.00 | 0.61 | -23.70 | 91.02 | -52.16 | 119.85 | 0.8359 | -447.0 | -404.6 | |
| 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. | |