| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.54 | 222.74 | 40.69 | 255.11 | 9.50 | 55.40 | -64.43 | 81.27 | 0.9002 | -484.8 | -157.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-07 04:58:59 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 | 0.43 | 0.00 | 0.45 | 10.84 | 57.77 | -62.06 | 79.72 | 0.8838 | 262.0 | 261.0 | |
| 20.29 | 196.14 | 21.85 | 213.62 | 9.23 | 57.01 | -62.83 | 81.56 | 0.8896 | -825.3 | -183.8 | |
| 0.00 | 0.26 | 0.00 | 0.28 | 10.61 | 56.53 | -63.31 | 80.01 | 0.8936 | -418.0 | -403.3 | |
| 1.90 | -2.00 | 2.06 | -2.00 | 8.82 | 56.73 | -63.10 | 82.02 | 0.8918 | -515.5 | 999999 | |
| 0.00 | 0.78 | 0.00 | 0.88 | 11.73 | 55.38 | -64.46 | 78.79 | 0.9024 | 196.0 | 298.6 | |
| 2.68 | -2.00 | 2.96 | -2.00 | 9.30 | 56.24 | -63.59 | 81.48 | 0.8956 | -220.3 | 999999 | |
| 2.16 | -2.00 | 2.39 | -2.00 | 9.54 | 56.16 | -63.67 | 81.22 | 0.8962 | -232.2 | 999999 | |
| 5.09 | 12.35 | 7.26 | 17.66 | 9.79 | 49.85 | -69.98 | 80.95 | 0.9391 | -499.7 | -269.5 | |
| 0.95 | -8.00 | 1.37 | -8.00 | 9.81 | 49.58 | -70.26 | 80.93 | 0.9407 | 184.8 | 999999 | |
| 0.00 | 3.80 | 0.00 | 5.48 | 9.23 | 49.57 | -70.26 | 81.54 | 0.9408 | -361.0 | -269.2 | |
| 0.00 | 1.38 | 0.00 | 2.42 | 12.24 | 45.77 | -74.06 | 78.34 | 0.9608 | 341.0 | 314.1 | |
| 0.00 | 1.99 | 0.00 | 3.66 | 12.52 | 44.96 | -74.87 | 78.04 | 0.9645 | 191.0 | 222.0 | |
| 1.47 | 5.61 | 2.80 | 10.66 | 12.65 | 44.50 | -75.34 | 77.91 | 0.9665 | 296.3 | 270.7 | |
| 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. | |