| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.11 | 280.52 | 22.51 | 153.43 | -24.50 | 250.01 | 14.59 | 212.72 | 0.4254 | 808.5 | 349.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2013-01-07 22:58:54 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 |
| 41.11 | 264.73 | 22.51 | 144.98 | -24.50 | 250.43 | 15.01 | 213.57 | 0.4281 | 1369.2 | 399.8 | |
| 0.00 | 2.80 | 0.00 | 1.52 | -24.98 | 247.94 | 12.52 | 208.48 | 0.4140 | 1014.0 | 772.1 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -28.04 | 245.38 | 9.97 | 200.39 | 0.4405 | -681.0 | -579.9 | |
| 0.00 | 1.02 | 0.00 | 0.55 | -26.63 | 244.86 | 9.44 | 200.68 | 0.4171 | -892.0 | -723.6 | |
| 0.00 | 1.70 | 0.00 | 0.90 | -22.94 | 244.52 | 9.10 | 203.93 | 0.3608 | -1003.0 | -819.2 | |
| 0.00 | 1.61 | 0.00 | 0.87 | -26.21 | 241.47 | 6.06 | 193.95 | 0.3945 | -784.0 | -582.3 | |
| 0.00 | 2.97 | 0.00 | 1.55 | -21.63 | 240.89 | 5.47 | 196.15 | 0.3201 | -777.0 | -731.3 | |
| 0.00 | 0.68 | 0.00 | 0.36 | -22.78 | 240.86 | 5.45 | 195.08 | 0.3382 | -716.0 | -602.0 | |
| 0.00 | 1.53 | 0.00 | 0.80 | -21.69 | 240.63 | 5.22 | 195.39 | 0.3200 | -872.0 | -693.7 | |
| 0.00 | 2.12 | 0.00 | 1.15 | -27.47 | 238.04 | 2.63 | 185.79 | 0.4050 | -633.0 | -349.6 | |
| 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. | |