| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.93 | 238.55 | 19.49 | 129.34 | 16.73 | 168.93 | 21.07 | 301.92 | 0.4075 | -720.5 | -366.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-19 00:59:11 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 |
| 27.58 | 230.10 | 14.97 | 124.85 | 16.66 | 169.16 | 21.30 | 301.47 | 0.4097 | -1209.4 | -407.2 | |
| 7.44 | -1.00 | 4.03 | -1.00 | 16.38 | 169.02 | 21.17 | 301.01 | 0.4059 | -1409.4 | 999999 | |
| 0.91 | -1.00 | 0.49 | -1.00 | 17.04 | 168.86 | 21.00 | 302.62 | 0.4086 | -917.6 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 20.48 | 166.00 | 18.14 | 313.45 | 0.4034 | 785.0 | 634.3 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 21.66 | 166.04 | 18.19 | 315.57 | 0.4161 | 804.0 | 622.1 | |
| 0.00 | 0.64 | 0.00 | 0.33 | 15.11 | 165.17 | 17.32 | 302.74 | 0.3431 | 687.0 | 489.3 | |
| 0.00 | 2.36 | 0.00 | 1.25 | 18.70 | 163.71 | 15.85 | 313.49 | 0.3581 | 637.0 | 515.7 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 17.59 | 162.77 | 14.92 | 312.68 | 0.3352 | 756.0 | 547.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 21.98 | 161.30 | 13.45 | 324.26 | 0.3707 | 818.0 | 658.8 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 20.28 | 160.48 | 12.62 | 322.89 | 0.3412 | 860.0 | 650.2 | |
| 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. | |