| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.37 | 91.46 | 14.72 | 50.94 | 13.54 | 291.66 | 26.98 | 285.73 | 0.4602 | -556.3 | -442.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-09-02 15:59:07 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 | 1.61 | 0.00 | 0.91 | 14.28 | 293.64 | 28.96 | 286.45 | 0.4912 | -733.0 | -573.4 | |
| 0.00 | 1.16 | 0.00 | 0.66 | 13.96 | 293.45 | 28.77 | 285.86 | 0.4875 | -647.0 | -500.5 | |
| 0.00 | 1.25 | 0.00 | 0.71 | 13.51 | 293.25 | 28.57 | 285.02 | 0.4834 | -418.0 | -411.6 | |
| 0.27 | 54.18 | 0.15 | 30.20 | 13.17 | 292.29 | 27.61 | 284.65 | 0.4683 | -728.0 | -588.6 | |
| 5.36 | -4.00 | 3.00 | -4.00 | 13.27 | 292.09 | 27.41 | 284.93 | 0.4656 | -977.6 | 999999 | |
| 3.93 | -4.00 | 2.19 | -4.00 | 13.10 | 291.83 | 27.14 | 284.67 | 0.4612 | -973.2 | 999999 | |
| 4.11 | 14.84 | 2.30 | 8.29 | 13.99 | 291.90 | 27.22 | 286.52 | 0.4648 | -971.0 | -567.6 | |
| 9.84 | 10.91 | 5.49 | 6.09 | 13.56 | 291.81 | 27.13 | 285.66 | 0.4623 | -1009.9 | -802.0 | |
| 2.86 | -4.00 | 1.59 | -4.00 | 13.21 | 291.56 | 26.88 | 285.00 | 0.4575 | -1132.5 | 999999 | |
| 0.00 | 1.79 | 0.00 | 0.98 | 11.26 | 290.42 | 25.74 | 281.04 | 0.4357 | 932.0 | 635.5 | |
| 0.00 | 1.97 | 0.00 | 1.07 | 14.89 | 288.07 | 23.39 | 290.55 | 0.4114 | 1035.0 | 812.3 | |
| 0.00 | 1.25 | 0.00 | 0.68 | 16.35 | 286.91 | 22.23 | 294.84 | 0.4017 | 722.0 | 628.7 | |
| 0.00 | 1.52 | 0.00 | 0.82 | 16.67 | 286.78 | 22.10 | 295.68 | 0.4016 | 600.0 | 574.5 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 16.75 | 286.38 | 21.70 | 296.22 | 0.3963 | 794.0 | 600.8 | |
| 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. | |