| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.26 | 306.28 | 51.46 | 174.38 | -21.11 | 53.45 | -9.77 | 161.39 | 0.4968 | -137.9 | -39.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-08-21 15:59:09 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 | 1.08 | 0.00 | 0.59 | -17.04 | 59.01 | -4.21 | 170.17 | 0.4132 | 781.0 | 682.2 | |
| 0.00 | 1.98 | 0.00 | 1.08 | -17.15 | 58.12 | -5.11 | 168.20 | 0.4176 | 772.0 | 641.4 | |
| 0.00 | 2.16 | 0.00 | 1.18 | -17.32 | 57.86 | -5.37 | 167.71 | 0.4211 | 793.0 | 633.3 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -17.42 | 57.60 | -5.62 | 167.19 | 0.4235 | 913.0 | 706.3 | |
| 2.52 | 72.27 | 1.43 | 41.02 | -21.78 | 56.65 | -6.57 | 167.50 | 0.4927 | 667.3 | 434.7 | |
| 13.57 | -5.00 | 7.70 | -5.00 | -21.47 | 56.44 | -6.78 | 166.95 | 0.4889 | 1160.7 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -19.09 | 55.99 | -7.23 | 164.78 | 0.4550 | 685.0 | 519.5 | |
| 0.90 | 3.60 | 0.51 | 2.05 | -21.97 | 55.76 | -7.47 | 165.95 | 0.4986 | 832.5 | 554.9 | |
| 1.17 | 15.01 | 0.66 | 8.49 | -20.47 | 54.85 | -8.37 | 163.43 | 0.4802 | 885.0 | 710.2 | |
| 10.61 | -9.00 | 6.00 | -9.00 | -20.68 | 54.64 | -8.58 | 163.18 | 0.4842 | 877.3 | 999999 | |
| 2.97 | 4.40 | 1.68 | 2.50 | -21.09 | 54.52 | -8.70 | 163.21 | 0.4908 | 736.5 | 578.6 | |
| 0.00 | 1.17 | 0.00 | 0.65 | -19.59 | 54.61 | -8.62 | 162.39 | 0.4684 | 699.0 | 493.7 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -21.17 | 54.25 | -8.97 | 162.78 | 0.4930 | 604.0 | 525.4 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -20.08 | 53.96 | -9.27 | 161.51 | 0.4786 | -735.0 | -548.4 | |
| 1.98 | 4.67 | 1.13 | 2.67 | -21.45 | 53.81 | -9.42 | 162.16 | 0.4992 | 773.1 | 420.8 | |
| 4.31 | 186.26 | 2.44 | 106.33 | -20.43 | 53.51 | -9.71 | 160.93 | 0.4859 | 829.5 | -305.2 | |
| 3.87 | -16.00 | 2.20 | -16.00 | -20.98 | 53.38 | -9.85 | 161.08 | 0.4945 | -798.8 | 999999 | |
| 0.00 | 1.71 | 0.00 | 0.96 | -19.92 | 53.21 | -10.01 | 160.02 | 0.4802 | -811.0 | -650.5 | |
| 1.71 | -16.00 | 0.98 | -16.00 | -21.37 | 52.95 | -10.27 | 160.61 | 0.5021 | -820.7 | 999999 | |
| 5.93 | -16.00 | 3.40 | -16.00 | -21.42 | 52.19 | -11.04 | 159.32 | 0.5068 | -855.4 | 999999 | |
| 1.53 | -16.00 | 0.87 | -16.00 | -21.04 | 52.22 | -11.01 | 159.09 | 0.5013 | -902.0 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -22.08 | 51.90 | -11.32 | 159.33 | 0.5175 | -556.0 | -418.8 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -21.63 | 51.87 | -11.35 | 158.95 | 0.5114 | -617.0 | -458.2 | |
| 30.11 | -16.00 | 17.24 | -16.00 | -21.02 | 51.79 | -11.44 | 158.33 | 0.5033 | -1063.6 | 999999 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -21.65 | 51.30 | -11.92 | 158.01 | 0.5148 | -524.0 | -431.2 | |
| 8.00 | -16.00 | 4.60 | -16.00 | -21.24 | 51.27 | -11.95 | 157.63 | 0.5093 | -872.7 | 999999 | |
| 1.08 | 1.71 | 0.62 | 0.98 | -21.48 | 51.05 | -12.17 | 157.46 | 0.5139 | -576.1 | -531.3 | |
| 0.00 | 1.08 | 0.00 | 0.63 | -22.11 | 50.73 | -12.50 | 157.43 | 0.5244 | -687.0 | -531.0 | |
| 0.00 | 1.08 | 0.00 | 0.65 | -24.91 | 48.83 | -14.39 | 156.71 | 0.5723 | -686.0 | -491.1 | |
| 0.00 | 0.54 | 0.00 | 0.32 | -24.67 | 48.80 | -14.43 | 156.47 | 0.5693 | -772.0 | -641.7 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -24.39 | 48.45 | -14.77 | 155.76 | 0.5678 | -500.0 | -460.0 | |
| 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. | |