| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.66 | 0.00 | 7.89 | 8.89 | 338.70 | -30.81 | 84.47 | 0.5080 | -372.7 | -253.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-17 00:00:35 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 | 1.33 | 0.00 | 0.72 | 9.58 | 345.05 | -24.45 | 82.64 | 0.4133 | 699.0 | 543.5 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 7.84 | 343.05 | -26.46 | 86.84 | 0.4439 | -814.0 | -620.9 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 8.92 | 342.90 | -26.60 | 84.41 | 0.4463 | -807.0 | -671.5 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 7.39 | 342.98 | -26.53 | 87.87 | 0.4451 | -760.0 | -599.5 | |
| 0.00 | 1.15 | 0.00 | 0.64 | 8.51 | 341.94 | -27.56 | 85.38 | 0.4610 | -783.0 | -555.5 | |
| 0.00 | 0.80 | 0.00 | 0.45 | 10.25 | 341.69 | -27.82 | 81.63 | 0.4660 | -820.0 | -669.4 | |
| 0.00 | 2.57 | 0.00 | 1.44 | 10.38 | 341.33 | -28.18 | 81.41 | 0.4716 | -676.0 | -576.4 | |
| 0.00 | 0.53 | 0.00 | 0.30 | 6.85 | 339.91 | -29.59 | 88.80 | 0.4924 | -640.0 | -529.7 | |
| 0.00 | 0.71 | 0.00 | 0.41 | 9.67 | 338.65 | -30.85 | 83.15 | 0.5112 | -453.0 | -496.8 | |
| 0.00 | 0.71 | 0.00 | 0.42 | 9.22 | 335.47 | -34.03 | 84.15 | 0.5575 | -620.0 | -525.4 | |
| 0.00 | 0.53 | 0.00 | 0.32 | 10.55 | 333.70 | -35.80 | 81.89 | 0.5831 | -376.0 | -438.5 | |
| 0.00 | 1.15 | 0.00 | 0.74 | 7.86 | 329.74 | -39.77 | 86.35 | 0.6372 | 523.0 | 545.3 | |
| 0.00 | 1.24 | 0.00 | 0.83 | 7.33 | 327.29 | -42.21 | 87.02 | 0.6696 | 682.0 | 530.6 | |
| 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. | |