| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.27 | 222.59 | 18.45 | 123.64 | -24.62 | 283.70 | 2.16 | 184.41 | 0.4536 | 369.0 | 254.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-22 05:58:57 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 | 0.94 | 0.00 | 0.52 | -23.98 | 287.53 | 5.99 | 192.27 | 0.4504 | 650.0 | 601.0 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -25.53 | 285.26 | 3.72 | 187.22 | 0.4682 | 325.0 | 287.8 | |
| 29.67 | 183.76 | 16.46 | 102.05 | -24.60 | 284.75 | 3.21 | 186.48 | 0.4528 | 1361.3 | 406.4 | |
| 0.00 | 3.00 | 0.00 | 1.64 | -23.15 | 283.71 | 2.17 | 184.68 | 0.4285 | 701.0 | 749.2 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -23.37 | 283.36 | 1.82 | 183.89 | 0.4317 | 616.0 | 442.2 | |
| 2.23 | 2.57 | 1.23 | 1.42 | -23.93 | 283.21 | 1.67 | 183.47 | 0.4404 | 816.5 | 684.0 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -21.97 | 280.85 | -0.69 | 178.43 | 0.4086 | 764.0 | 640.1 | |
| 0.00 | 1.29 | 0.00 | 0.71 | -23.54 | 280.68 | -0.86 | 178.18 | 0.4336 | -857.0 | -682.1 | |
| 0.00 | 3.26 | 0.00 | 1.79 | -23.90 | 280.65 | -0.89 | 178.13 | 0.4393 | -770.0 | -724.2 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -24.59 | 279.60 | -1.94 | 176.07 | 0.4510 | -764.0 | -639.1 | |
| 0.00 | 1.37 | 0.00 | 0.77 | -26.03 | 277.59 | -3.94 | 172.51 | 0.4763 | -659.0 | -430.9 | |
| 0.00 | 1.11 | 0.00 | 0.62 | -25.47 | 277.25 | -4.29 | 171.68 | 0.4684 | -814.0 | -537.9 | |
| 1.37 | 2.06 | 0.76 | 1.13 | -23.54 | 277.16 | -4.38 | 170.78 | 0.4390 | -911.6 | -838.0 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -26.64 | 277.01 | -4.53 | 171.63 | 0.4868 | -590.0 | -518.2 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -26.41 | 276.79 | -4.75 | 171.14 | 0.4838 | -859.0 | -778.0 | |
| 0.00 | 2.14 | 0.00 | 1.18 | -23.35 | 276.32 | -5.22 | 168.97 | 0.4383 | -778.0 | -626.4 | |
| 0.00 | 2.06 | 0.00 | 1.17 | -27.29 | 276.11 | -5.43 | 170.26 | 0.4987 | -831.0 | -609.7 | |
| 0.00 | 2.40 | 0.00 | 1.35 | -25.94 | 276.11 | -5.43 | 169.71 | 0.4784 | -1025.0 | -811.8 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -26.21 | 276.07 | -5.47 | 169.74 | 0.4826 | -504.0 | -526.2 | |
| 0.00 | 5.57 | 0.00 | 3.15 | -26.31 | 275.73 | -5.81 | 169.17 | 0.4851 | -937.0 | -800.4 | |
| 0.00 | 0.69 | 0.00 | 0.38 | -24.08 | 275.57 | -5.97 | 167.83 | 0.4518 | -895.0 | -696.6 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -24.37 | 275.46 | -6.08 | 167.76 | 0.4567 | -743.0 | -631.0 | |
| 0.00 | 1.46 | 0.00 | 0.80 | -22.60 | 274.96 | -6.58 | 165.76 | 0.4316 | -562.0 | -583.6 | |
| 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. | |