| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.54 | 52.72 | 5.67 | 28.44 | 17.74 | 325.07 | -20.04 | 56.14 | 0.3944 | 319.8 | 136.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-10-21 02:59:01 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 | 1.39 | 0.00 | 0.72 | 10.13 | 330.61 | -14.50 | 71.00 | 0.2618 | 723.0 | 575.1 | |
| 0.00 | 1.66 | 0.00 | 0.87 | 15.52 | 329.13 | -15.97 | 56.04 | 0.3211 | 874.0 | 664.5 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 14.66 | 327.65 | -17.45 | 60.44 | 0.3351 | 924.0 | 743.8 | |
| 0.00 | 1.13 | 0.00 | 0.60 | 17.51 | 327.23 | -17.88 | 53.90 | 0.3640 | -838.0 | -578.0 | |
| 0.00 | 2.61 | 0.00 | 1.39 | 17.84 | 327.16 | -17.95 | 53.22 | 0.3678 | -854.0 | -786.0 | |
| 1.48 | 13.42 | 0.79 | 7.14 | 17.68 | 326.95 | -18.16 | 53.89 | 0.3692 | -901.3 | -569.5 | |
| 3.14 | -6.00 | 1.67 | -6.00 | 17.31 | 326.82 | -18.29 | 54.92 | 0.3677 | -900.3 | 999999 | |
| 1.31 | 2.96 | 0.70 | 1.58 | 17.00 | 326.49 | -18.62 | 56.09 | 0.3695 | -813.5 | -774.4 | |
| 0.00 | 1.13 | 0.00 | 0.61 | 17.97 | 326.32 | -18.79 | 54.09 | 0.3799 | 622.0 | 496.9 | |
| 0.00 | 1.66 | 0.00 | 0.89 | 17.01 | 325.83 | -19.28 | 56.91 | 0.3785 | -125.0 | -261.6 | |
| 2.09 | 5.23 | 1.12 | 2.81 | 18.17 | 325.63 | -19.47 | 54.55 | 0.3905 | 868.8 | 705.0 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 16.91 | 325.54 | -19.57 | 57.50 | 0.3816 | 697.0 | 570.9 | |
| 0.00 | 1.48 | 0.00 | 0.80 | 17.35 | 324.96 | -20.15 | 57.19 | 0.3929 | 826.0 | 499.4 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 18.41 | 324.60 | -20.51 | 55.29 | 0.4061 | 1128.0 | 866.5 | |
| 0.00 | 2.44 | 0.00 | 1.32 | 17.55 | 324.64 | -20.47 | 57.11 | 0.3988 | 593.0 | 618.2 | |
| 0.00 | 2.79 | 0.00 | 1.51 | 18.52 | 324.32 | -20.79 | 55.39 | 0.4107 | 791.0 | 675.5 | |
| 1.13 | 4.53 | 0.62 | 2.49 | 19.24 | 322.86 | -22.25 | 55.54 | 0.4354 | 1113.5 | 895.3 | |
| 1.39 | -17.00 | 0.77 | -17.00 | 19.42 | 322.77 | -22.34 | 55.27 | 0.4380 | 793.2 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 21.39 | 320.61 | -24.50 | 53.77 | 0.4806 | 620.0 | 609.6 | |
| 0.00 | 0.87 | 0.00 | 0.49 | 20.40 | 320.61 | -24.50 | 55.60 | 0.4731 | 798.0 | 550.2 | |
| 0.00 | 1.39 | 0.00 | 0.79 | 20.60 | 319.51 | -25.59 | 56.23 | 0.4884 | 769.0 | 616.5 | |
| 0.00 | 1.22 | 0.00 | 0.69 | 20.20 | 319.48 | -25.63 | 57.00 | 0.4860 | 759.0 | 604.2 | |
| 0.00 | 1.05 | 0.00 | 0.59 | 19.74 | 318.85 | -26.25 | 58.38 | 0.4909 | 587.0 | 441.2 | |
| 0.00 | 1.74 | 0.00 | 0.98 | 16.09 | 318.11 | -27.00 | 65.93 | 0.4796 | -813.0 | -569.4 | |
| 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. | |