| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.76 | 196.11 | 19.66 | 121.05 | 16.89 | 168.79 | 35.27 | 292.15 | 0.5987 | -536.3 | -299.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-20 02:59:11 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 | 0.64 | 0.00 | 0.39 | 12.26 | 169.13 | 35.61 | 284.35 | 0.5895 | -650.0 | -567.6 | |
| 0.91 | 182.21 | 0.56 | 112.79 | 17.11 | 169.27 | 35.75 | 292.26 | 0.6055 | -567.0 | -374.3 | |
| 30.85 | -2.00 | 19.10 | -2.00 | 16.71 | 169.10 | 35.58 | 291.69 | 0.6019 | -1097.5 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.72 | 21.14 | 166.75 | 33.22 | 299.95 | 0.5919 | 660.0 | 464.2 | |
| 0.00 | 1.81 | 0.00 | 1.11 | 21.48 | 166.25 | 32.72 | 300.80 | 0.5877 | 627.0 | 596.3 | |
| 0.00 | 1.45 | 0.00 | 0.88 | 22.32 | 165.56 | 32.04 | 302.54 | 0.5843 | 815.0 | 640.5 | |
| 0.00 | 1.00 | 0.00 | 0.59 | 18.50 | 164.05 | 30.52 | 297.26 | 0.5439 | 652.0 | 552.3 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 18.40 | 163.40 | 29.87 | 297.50 | 0.5349 | 661.0 | 597.8 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 18.78 | 163.36 | 29.83 | 298.19 | 0.5364 | 457.0 | 515.6 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 17.38 | 162.91 | 29.39 | 296.00 | 0.5231 | 702.0 | 536.8 | |
| 0.00 | 4.36 | 0.00 | 2.55 | 18.69 | 163.12 | 29.59 | 298.20 | 0.5329 | 649.0 | 654.5 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 18.48 | 162.86 | 29.33 | 298.00 | 0.5283 | 798.0 | 715.0 | |
| 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. | |