SDO HMI 2011-06-14 21:59:11 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.75 | 410.23 | 149.24 | 751.21 | 16.38 | 165.73 | -73.79 | 73.19 | 0.9614 | 64.5 | -41.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-06-14 21:59:11 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 |
| 17.40 | 196.55 | 24.57 | 281.07 | 16.93 | 170.72 | -68.81 | 72.25 | 0.9380 | -748.3 | -153.0 | |
| 4.08 | -1.00 | 5.88 | -1.00 | 17.12 | 170.30 | -69.23 | 72.10 | 0.9405 | 244.2 | 999999 | |
| 11.60 | -1.00 | 16.67 | -1.00 | 16.32 | 170.30 | -69.23 | 72.94 | 0.9401 | -559.7 | 999999 | |
| 3.26 | -1.00 | 4.77 | -1.00 | 16.51 | 169.97 | -69.56 | 72.77 | 0.9420 | 353.2 | 999999 | |
| 0.00 | 2.72 | 0.00 | 4.25 | 17.03 | 168.57 | -70.95 | 72.35 | 0.9499 | 432.0 | 362.1 | |
| 0.00 | 9.61 | 0.00 | 15.77 | 17.21 | 167.59 | -71.93 | 72.24 | 0.9549 | 346.0 | 243.4 | |
| 0.00 | 0.72 | 0.00 | 1.14 | 15.18 | 168.36 | -71.16 | 74.30 | 0.9502 | -151.0 | -133.9 | |
| 0.00 | 1.00 | 0.00 | 1.42 | 11.95 | 170.10 | -69.43 | 77.60 | 0.9393 | -359.0 | -331.5 | |
| 0.00 | 1.00 | 0.00 | 1.57 | 14.58 | 168.24 | -71.28 | 74.94 | 0.9506 | -177.0 | -203.2 | |
| 0.00 | 0.91 | 0.00 | 1.76 | 17.71 | 164.67 | -74.85 | 71.93 | 0.9683 | 531.0 | 492.0 | |
| 0.00 | 5.07 | 0.00 | 10.77 | 18.59 | 163.41 | -76.12 | 71.11 | 0.9736 | 359.0 | 300.1 | |
| 4.26 | 84.09 | 9.70 | 195.98 | 18.12 | 162.37 | -77.16 | 71.64 | 0.9773 | 461.1 | 82.4 | |
| 0.00 | 1.36 | 0.00 | 2.76 | 16.80 | 163.97 | -75.55 | 72.91 | 0.9710 | 490.0 | 412.1 | |
| 0.00 | 1.99 | 0.00 | 3.69 | 15.27 | 165.38 | -74.14 | 74.41 | 0.9646 | 246.0 | 266.5 | |
| 12.78 | -12.00 | 29.14 | -12.00 | 17.32 | 162.34 | -77.19 | 72.46 | 0.9772 | 514.8 | 999999 | |
| 0.00 | 2.72 | 0.00 | 5.81 | 16.69 | 163.17 | -76.36 | 73.06 | 0.9741 | 562.0 | 507.9 | |
| 0.54 | 6.62 | 1.04 | 12.85 | 15.07 | 164.74 | -74.79 | 74.65 | 0.9674 | -339.3 | -79.7 | |
| 0.00 | 3.44 | 0.00 | 6.79 | 15.32 | 164.36 | -75.16 | 74.42 | 0.9690 | 450.0 | 392.8 | |
| 1.54 | -17.00 | 3.02 | -17.00 | 14.97 | 164.47 | -75.06 | 74.77 | 0.9685 | -292.3 | 999999 | |
| 3.99 | -12.00 | 9.31 | -12.00 | 16.77 | 162.06 | -77.46 | 73.04 | 0.9781 | 369.0 | 999999 | |
| 1.00 | -17.00 | 1.99 | -17.00 | 15.00 | 164.19 | -75.34 | 74.75 | 0.9697 | 317.5 | 999999 | |
| 4.53 | -12.00 | 10.43 | -12.00 | 16.17 | 162.27 | -77.25 | 73.64 | 0.9772 | 342.3 | 999999 | |
| 4.89 | 57.27 | 10.42 | 119.69 | 14.92 | 163.22 | -76.30 | 74.88 | 0.9735 | 482.1 | -33.1 | |
| 0.00 | 0.91 | 0.00 | 2.36 | 16.79 | 160.78 | -78.75 | 73.08 | 0.9823 | -432.0 | -412.4 | |
| 3.17 | -23.00 | 6.60 | -23.00 | 14.70 | 163.46 | -76.06 | 75.09 | 0.9725 | -287.7 | 999999 | |
| 0.00 | 1.81 | 0.00 | 4.71 | 16.63 | 160.69 | -78.83 | 73.25 | 0.9826 | -391.0 | -373.9 | |
| 6.71 | 29.90 | 15.70 | 72.29 | 15.44 | 161.89 | -77.64 | 74.41 | 0.9785 | 327.4 | -143.6 | |
| 0.00 | 1.54 | 0.00 | 3.94 | 16.02 | 160.93 | -78.60 | 73.85 | 0.9818 | -457.0 | -414.2 | |
| 0.00 | 1.00 | 0.00 | 2.59 | 16.15 | 160.74 | -78.78 | 73.73 | 0.9824 | -408.0 | -364.3 | |
| 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. | |