| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.15 | 43.65 | 17.58 | 41.63 | 17.30 | 133.47 | 56.75 | 290.73 | 0.8497 | 226.9 | -126.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-07 18:58:56 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 |
| 4.26 | 11.76 | 4.76 | 13.10 | 16.83 | 139.10 | 62.38 | 288.81 | 0.8978 | -214.6 | -346.4 | |
| 0.00 | 0.94 | 0.00 | 1.01 | 17.02 | 137.96 | 61.23 | 289.21 | 0.8895 | -269.0 | -196.2 | |
| 8.69 | 14.83 | 8.99 | 15.36 | 16.40 | 136.80 | 60.08 | 288.71 | 0.8798 | 455.9 | 10.2 | |
| 0.00 | 2.05 | 0.00 | 1.65 | 18.45 | 126.43 | 49.71 | 293.56 | 0.7917 | -615.0 | -486.1 | |
| 0.00 | 2.05 | 0.00 | 1.61 | 19.57 | 124.97 | 48.25 | 295.42 | 0.7805 | -627.0 | -577.8 | |
| 0.00 | 0.94 | 0.00 | 0.74 | 19.70 | 124.83 | 48.11 | 295.62 | 0.7796 | -551.0 | -487.1 | |
| 5.20 | 8.10 | 3.83 | 5.96 | 18.23 | 121.69 | 44.97 | 294.91 | 0.7425 | 721.5 | 481.6 | |
| 0.00 | 1.02 | 0.00 | 0.76 | 20.26 | 121.25 | 44.53 | 297.70 | 0.7454 | 443.0 | 297.7 | |
| 0.00 | 0.85 | 0.00 | 0.63 | 20.80 | 120.79 | 44.06 | 298.58 | 0.7427 | 653.0 | 568.9 | |
| 0.00 | 1.11 | 0.00 | 0.81 | 20.93 | 120.66 | 43.93 | 298.79 | 0.7418 | 703.0 | 571.8 | |
| 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. | |