| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.40 | 69.91 | 8.43 | 40.74 | 13.70 | 291.34 | 31.62 | 284.50 | 0.5283 | -256.1 | -357.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-09-03 00:59:07 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 |
| 4.83 | 52.31 | 2.83 | 30.62 | 13.21 | 292.14 | 32.43 | 283.29 | 0.5385 | -788.9 | -542.9 | |
| 6.08 | -1.00 | 3.56 | -1.00 | 13.53 | 291.93 | 32.22 | 283.93 | 0.5361 | -841.2 | 999999 | |
| 0.00 | 5.81 | 0.00 | 3.41 | 14.02 | 291.90 | 32.18 | 284.85 | 0.5367 | -849.0 | -763.1 | |
| 3.49 | -1.00 | 2.04 | -1.00 | 13.18 | 291.59 | 31.87 | 283.38 | 0.5305 | -1023.4 | 999999 | |
| 0.00 | 1.43 | 0.00 | 0.83 | 13.35 | 291.32 | 31.60 | 283.77 | 0.5270 | -410.0 | -379.9 | |
| 0.00 | 0.98 | 0.00 | 0.57 | 11.46 | 290.92 | 31.20 | 280.23 | 0.5180 | 638.0 | 485.8 | |
| 0.00 | 1.79 | 0.00 | 1.02 | 15.52 | 288.42 | 28.71 | 288.98 | 0.4914 | 749.0 | 563.5 | |
| 0.00 | 0.80 | 0.00 | 0.46 | 14.92 | 288.23 | 28.51 | 287.86 | 0.4866 | 756.0 | 595.8 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 15.86 | 287.97 | 28.26 | 289.86 | 0.4862 | 762.0 | 661.1 | |
| 0.00 | 1.79 | 0.00 | 1.01 | 15.77 | 287.85 | 28.14 | 289.74 | 0.4842 | 740.0 | 492.5 | |
| 0.00 | 4.02 | 0.00 | 2.26 | 16.37 | 287.05 | 27.34 | 291.37 | 0.4751 | 721.0 | 632.0 | |
| 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. | |