| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.92 | 53.47 | 15.82 | 191.30 | -11.19 | 306.39 | -80.64 | 101.88 | 0.9894 | -113.3 | -376.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-09 06:00:27 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 | 1.12 | 0.00 | 1.66 | -11.47 | 317.85 | -69.19 | 103.50 | 0.9436 | 305.0 | 331.8 | |
| 1.64 | 3.71 | 3.58 | 8.11 | -11.62 | 311.17 | -75.86 | 102.80 | 0.9751 | 65.4 | 94.4 | |
| 0.00 | 0.86 | 0.00 | 2.22 | -12.42 | 309.20 | -77.83 | 103.39 | 0.9822 | 248.0 | 178.1 | |
| 0.69 | 7.76 | 2.16 | 25.92 | -13.28 | 307.21 | -79.82 | 104.05 | 0.9882 | 93.1 | -265.0 | |
| 0.00 | 0.60 | 0.00 | 2.23 | -13.70 | 305.81 | -81.22 | 104.34 | 0.9917 | -397.0 | -388.3 | |
| 0.00 | 1.55 | 0.00 | 4.72 | -11.85 | 307.44 | -79.59 | 102.64 | 0.9872 | -62.0 | -113.4 | |
| 0.00 | 5.09 | 0.00 | 19.50 | -12.19 | 305.46 | -81.57 | 102.79 | 0.9921 | -522.0 | -499.5 | |
| 0.78 | 26.91 | 2.67 | 103.11 | -10.68 | 306.07 | -80.96 | 101.33 | 0.9904 | -440.8 | -464.5 | |
| 0.00 | 0.69 | 0.00 | 2.86 | -10.74 | 304.71 | -82.32 | 101.27 | 0.9934 | -349.0 | -407.0 | |
| 1.81 | 5.18 | 7.41 | 20.97 | -9.49 | 304.80 | -82.24 | 100.02 | 0.9930 | -128.6 | -154.3 | |
| 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. | |