| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.74 | 329.65 | 33.30 | 203.98 | 12.02 | 275.18 | 32.51 | 298.65 | 0.6012 | -846.1 | -339.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-04-16 06:00:34 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 |
| 0.27 | 313.81 | 0.17 | 194.61 | 11.55 | 275.86 | 33.20 | 297.41 | 0.6065 | -691.0 | -379.3 | |
| 51.61 | -1.00 | 32.00 | -1.00 | 11.93 | 275.44 | 32.77 | 298.29 | 0.6037 | -1315.5 | 999999 | |
| 0.97 | -1.00 | 0.61 | -1.00 | 12.50 | 275.48 | 32.82 | 299.10 | 0.6078 | -685.4 | 999999 | |
| 0.00 | 1.68 | 0.00 | 1.04 | 15.09 | 273.29 | 30.62 | 304.59 | 0.5997 | -568.0 | -441.5 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 12.58 | 271.36 | 28.69 | 302.56 | 0.5581 | 608.0 | 456.6 | |
| 0.00 | 1.15 | 0.00 | 0.69 | 12.82 | 271.07 | 28.41 | 303.19 | 0.5564 | 628.0 | 518.5 | |
| 0.00 | 2.12 | 0.00 | 1.27 | 13.76 | 270.77 | 28.11 | 304.90 | 0.5601 | 640.0 | 472.0 | |
| 0.00 | 0.97 | 0.00 | 0.58 | 13.05 | 270.50 | 27.84 | 304.07 | 0.5513 | 716.0 | 528.8 | |
| 0.89 | 1.86 | 0.52 | 1.09 | 12.59 | 269.37 | 26.71 | 304.44 | 0.5340 | 706.8 | 561.3 | |
| 0.00 | 1.42 | 0.00 | 0.83 | 13.99 | 268.12 | 25.46 | 307.93 | 0.5309 | 843.0 | 717.9 | |
| 0.00 | 2.30 | 0.00 | 1.35 | 14.57 | 268.16 | 25.50 | 308.76 | 0.5364 | 656.0 | 367.6 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 16.36 | 267.08 | 24.42 | 312.57 | 0.5408 | 629.0 | 582.8 | |
| 0.00 | 0.97 | 0.00 | 0.56 | 13.61 | 266.51 | 23.85 | 309.14 | 0.5086 | 752.0 | 610.8 | |
| 0.00 | 1.42 | 0.00 | 0.81 | 13.70 | 266.42 | 23.75 | 309.39 | 0.5084 | 570.0 | 427.0 | |
| 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. | |