| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.81 | 12.54 | 0.50 | 7.75 | -20.32 | 157.97 | -25.53 | 137.25 | 0.5971 | 416.2 | 288.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-07 14:00:39 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 | 1.08 | 0.00 | 0.66 | -20.22 | 159.92 | -23.58 | 139.30 | 0.5779 | 696.0 | 580.7 | |
| 0.00 | 0.99 | 0.00 | 0.61 | -21.12 | 159.59 | -23.91 | 139.98 | 0.5902 | 589.0 | 434.5 | |
| 0.81 | 3.61 | 0.50 | 2.21 | -20.43 | 159.11 | -24.40 | 138.60 | 0.5876 | 890.3 | 672.8 | |
| 0.00 | 0.81 | 0.00 | 0.50 | -20.40 | 158.93 | -24.57 | 138.38 | 0.5890 | 736.0 | 657.2 | |
| 0.00 | 1.90 | 0.00 | 1.13 | -17.16 | 158.77 | -24.73 | 134.08 | 0.5586 | 504.0 | 322.5 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -20.30 | 158.16 | -25.34 | 137.40 | 0.5952 | 618.0 | 523.7 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -20.40 | 157.57 | -25.94 | 136.87 | 0.6018 | 512.0 | 424.9 | |
| 0.00 | 0.63 | 0.00 | 0.39 | -20.57 | 157.43 | -26.08 | 136.93 | 0.6048 | 438.0 | 358.6 | |
| 0.00 | 1.08 | 0.00 | 0.70 | -22.05 | 154.62 | -28.89 | 135.83 | 0.6449 | -505.0 | -466.9 | |
| 0.00 | 1.54 | 0.00 | 0.99 | -21.89 | 154.47 | -29.04 | 135.50 | 0.6448 | -553.0 | -464.7 | |
| 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. | |