| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 14.02 | 0.28 | 9.11 | -23.15 | 93.73 | -32.96 | 129.30 | 0.6485 | -213.8 | -266.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-29 00:00:25 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 | 1.62 | 0.00 | 1.01 | -23.28 | 97.77 | -28.91 | 132.83 | 0.6078 | 879.0 | 716.1 | |
| 0.00 | 0.77 | 0.00 | 0.50 | -23.77 | 94.84 | -31.84 | 130.94 | 0.6415 | 658.0 | 561.6 | |
| 0.43 | 1.62 | 0.28 | 1.05 | -23.51 | 94.76 | -31.92 | 130.54 | 0.6404 | 779.0 | 633.9 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -22.08 | 94.95 | -31.74 | 128.81 | 0.6278 | -784.0 | -593.3 | |
| 0.00 | 2.65 | 0.00 | 1.74 | -24.08 | 93.29 | -33.40 | 130.13 | 0.6595 | -587.0 | -583.9 | |
| 0.00 | 1.37 | 0.00 | 0.89 | -23.07 | 93.23 | -33.45 | 128.79 | 0.6529 | -572.0 | -458.7 | |
| 0.00 | 1.20 | 0.00 | 0.80 | -24.45 | 92.63 | -34.05 | 130.10 | 0.6688 | -723.0 | -632.7 | |
| 0.00 | 0.94 | 0.00 | 0.62 | -24.32 | 92.63 | -34.05 | 129.93 | 0.6678 | -676.0 | -581.6 | |
| 0.00 | 2.14 | 0.00 | 1.38 | -20.26 | 92.42 | -34.27 | 124.43 | 0.6427 | -852.0 | -671.5 | |
| 0.00 | 0.68 | 0.00 | 0.47 | -24.42 | 89.59 | -37.09 | 127.95 | 0.6987 | -538.0 | -498.4 | |
| 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. | |