| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 28.86 | 0.00 | 16.09 | -23.86 | 8.76 | 1.49 | 183.02 | 0.4603 | 653.1 | 572.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-11-10 18:00:27 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 | 0.86 | 0.00 | 0.47 | -20.74 | 10.12 | 2.85 | 186.50 | 0.4129 | 933.0 | 731.8 | |
| 0.00 | 1.81 | 0.00 | 1.00 | -22.28 | 10.05 | 2.79 | 185.93 | 0.4370 | 847.0 | 673.4 | |
| 0.00 | 1.72 | 0.00 | 0.94 | -21.98 | 9.41 | 2.14 | 184.62 | 0.4314 | 890.0 | 810.5 | |
| 0.00 | 2.84 | 0.00 | 1.58 | -23.30 | 9.36 | 2.09 | 184.28 | 0.4520 | 817.0 | 632.0 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -24.98 | 9.13 | 1.86 | 183.54 | 0.4777 | 713.0 | 616.7 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -23.77 | 9.04 | 1.78 | 183.56 | 0.4589 | 890.0 | 764.1 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -24.07 | 8.98 | 1.72 | 183.39 | 0.4635 | 776.0 | 658.0 | |
| 0.00 | 7.15 | 0.00 | 4.00 | -24.37 | 8.95 | 1.69 | 183.30 | 0.4682 | 720.0 | 637.4 | |
| 0.00 | 3.19 | 0.00 | 1.79 | -24.81 | 8.96 | 1.69 | 183.25 | 0.4749 | 729.0 | 609.0 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -23.94 | 8.75 | 1.49 | 182.96 | 0.4613 | 972.0 | 864.2 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -24.30 | 8.47 | 1.20 | 182.35 | 0.4668 | 627.0 | 555.9 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -24.67 | 8.17 | 0.91 | 181.75 | 0.4723 | 650.0 | 518.4 | |
| 0.00 | 3.88 | 0.00 | 2.16 | -23.77 | 7.75 | 0.48 | 180.96 | 0.4581 | 385.0 | 350.1 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -25.24 | 4.73 | -2.54 | 175.22 | 0.4825 | -805.0 | -622.9 | |
| 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. | |