| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.75 | 165.98 | 46.99 | 262.44 | 15.36 | 88.57 | 73.00 | 283.87 | 0.9512 | 327.5 | 129.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-16 13:00:35 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 |
| 20.78 | 127.80 | 33.09 | 203.18 | 14.84 | 88.66 | 73.09 | 283.32 | 0.9518 | 503.9 | 160.4 | |
| 1.42 | 9.95 | 2.36 | 16.39 | 16.58 | 89.56 | 73.99 | 285.19 | 0.9559 | -434.0 | 27.5 | |
| 1.33 | -2.00 | 2.20 | -2.00 | 16.79 | 89.43 | 73.86 | 285.40 | 0.9552 | -44.6 | 999999 | |
| 0.00 | 3.73 | 0.00 | 6.04 | 17.37 | 89.03 | 73.45 | 285.99 | 0.9531 | 164.0 | 174.1 | |
| 0.00 | 2.04 | 0.00 | 3.25 | 18.12 | 88.83 | 73.26 | 286.78 | 0.9520 | -435.0 | -401.2 | |
| 4.62 | 7.37 | 6.93 | 11.03 | 17.20 | 87.56 | 71.98 | 285.76 | 0.9454 | 434.0 | 273.5 | |
| 0.00 | 4.26 | 0.00 | 6.20 | 16.61 | 86.91 | 71.33 | 285.12 | 0.9419 | 505.0 | 395.7 | |
| 1.60 | 3.46 | 2.41 | 5.24 | 17.56 | 87.70 | 72.13 | 286.15 | 0.9461 | 391.2 | 282.0 | |
| 0.00 | 1.33 | 0.00 | 2.12 | 18.60 | 88.81 | 73.24 | 287.28 | 0.9518 | -635.0 | -514.0 | |
| 0.00 | 2.40 | 0.00 | 3.77 | 18.32 | 88.50 | 72.92 | 286.98 | 0.9502 | -522.0 | -496.4 | |
| 0.00 | 1.42 | 0.00 | 2.26 | 18.76 | 88.77 | 73.20 | 287.45 | 0.9515 | -440.0 | -342.6 | |
| 0.00 | 1.07 | 0.00 | 1.47 | 15.95 | 85.58 | 70.01 | 284.38 | 0.9343 | 281.0 | 253.8 | |
| 0.00 | 1.15 | 0.00 | 1.49 | 13.59 | 83.92 | 68.34 | 281.78 | 0.9245 | -410.0 | -378.7 | |
| 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. | |