| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.17 | 150.51 | 16.68 | 80.47 | -11.22 | 180.27 | 13.21 | 216.65 | 0.3768 | 695.8 | 328.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-10-07 07:59:03 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 |
| 28.28 | 137.25 | 15.13 | 73.48 | -11.19 | 180.70 | 13.64 | 217.72 | 0.3798 | 1214.2 | 404.1 | |
| 1.40 | -1.00 | 0.75 | -1.00 | -11.14 | 180.13 | 13.08 | 216.62 | 0.3737 | 907.8 | 999999 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -10.89 | 180.03 | 12.97 | 216.81 | 0.3694 | 377.0 | 360.2 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -10.23 | 179.97 | 12.91 | 217.80 | 0.3603 | 800.0 | 607.8 | |
| 1.49 | 2.20 | 0.80 | 1.17 | -11.20 | 179.88 | 12.83 | 216.01 | 0.3721 | 956.4 | 804.2 | |
| 0.00 | 1.32 | 0.00 | 0.69 | -11.47 | 174.73 | 7.68 | 203.17 | 0.3343 | -848.0 | -686.5 | |
| 0.00 | 1.23 | 0.00 | 0.65 | -12.28 | 174.11 | 7.05 | 200.58 | 0.3428 | -921.0 | -785.9 | |
| 0.00 | 1.40 | 0.00 | 0.74 | -12.34 | 173.77 | 6.72 | 199.61 | 0.3418 | -1006.0 | -814.8 | |
| 0.00 | 1.05 | 0.00 | 0.55 | -12.08 | 173.21 | 6.15 | 198.33 | 0.3348 | -730.0 | -619.1 | |
| 0.00 | 3.25 | 0.00 | 1.70 | -11.92 | 172.84 | 5.78 | 197.43 | 0.3304 | -1013.0 | -818.4 | |
| 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. | |