| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.09 | 188.78 | 32.70 | 116.45 | -12.33 | 163.27 | 31.33 | 238.67 | 0.5964 | 195.5 | 146.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-05 00:00:32 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 | 1.58 | 0.00 | 1.02 | -10.38 | 167.91 | 35.97 | 244.98 | 0.6398 | 703.0 | 598.3 | |
| 0.00 | 0.79 | 0.00 | 0.50 | -12.16 | 165.95 | 34.01 | 241.12 | 0.6267 | 456.0 | 334.7 | |
| 0.00 | 0.70 | 0.00 | 0.45 | -13.27 | 165.97 | 34.03 | 239.57 | 0.6339 | 661.0 | 569.0 | |
| 0.00 | 0.97 | 0.00 | 0.61 | -11.88 | 165.62 | 33.67 | 241.27 | 0.6209 | -292.0 | -152.4 | |
| 25.49 | 93.96 | 15.98 | 58.94 | -12.37 | 164.88 | 32.93 | 240.03 | 0.6152 | 928.4 | 319.8 | |
| 1.05 | -5.00 | 0.66 | -5.00 | -11.62 | 164.52 | 32.57 | 240.85 | 0.6061 | 823.2 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.67 | -14.73 | 164.91 | 32.97 | 236.75 | 0.6315 | 642.0 | 553.7 | |
| 1.41 | 24.08 | 0.87 | 14.84 | -11.41 | 164.20 | 32.26 | 240.91 | 0.6009 | 835.8 | 645.1 | |
| 3.25 | 9.93 | 2.02 | 6.17 | -12.26 | 164.09 | 32.15 | 239.59 | 0.6052 | 937.4 | 653.6 | |
| 3.69 | -9.00 | 2.29 | -9.00 | -12.42 | 164.12 | 32.17 | 239.38 | 0.6065 | 839.6 | 999999 | |
| 2.02 | -8.00 | 1.25 | -8.00 | -11.74 | 163.95 | 32.01 | 240.24 | 0.6000 | 780.7 | 999999 | |
| 2.99 | -8.00 | 1.84 | -8.00 | -11.36 | 163.79 | 31.85 | 240.69 | 0.5956 | 969.3 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.79 | -15.91 | 164.38 | 32.43 | 234.72 | 0.6341 | 568.0 | 472.6 | |
| 1.14 | 2.81 | 0.71 | 1.74 | -12.22 | 163.58 | 31.64 | 239.24 | 0.5988 | 803.8 | 645.9 | |
| 0.00 | 0.62 | 0.00 | 0.37 | -9.95 | 163.31 | 31.36 | 242.45 | 0.5804 | -444.0 | -381.9 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -10.86 | 163.34 | 31.39 | 241.08 | 0.5867 | -490.0 | -399.6 | |
| 0.44 | 2.11 | 0.27 | 1.28 | -10.57 | 163.27 | 31.33 | 241.47 | 0.5840 | -704.6 | -575.0 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -10.10 | 163.18 | 31.24 | 242.13 | 0.5798 | -672.0 | -537.6 | |
| 0.00 | 2.64 | 0.00 | 1.60 | -10.25 | 163.13 | 31.18 | 241.85 | 0.5801 | -860.0 | -702.6 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -11.12 | 163.08 | 31.14 | 240.48 | 0.5853 | 202.0 | 142.0 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -12.32 | 163.16 | 31.22 | 238.75 | 0.5945 | 554.0 | 487.3 | |
| 0.53 | 2.46 | 0.32 | 1.49 | -10.69 | 162.61 | 30.66 | 240.76 | 0.5765 | -773.8 | -653.0 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -11.27 | 162.46 | 30.52 | 239.75 | 0.5787 | -280.0 | -227.8 | |
| 0.00 | 2.20 | 0.00 | 1.33 | -10.95 | 162.35 | 30.41 | 240.15 | 0.5751 | -778.0 | -604.1 | |
| 0.00 | 0.62 | 0.00 | 0.41 | -20.94 | 163.63 | 31.69 | 227.76 | 0.6650 | 661.0 | 524.0 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -14.38 | 161.94 | 30.00 | 234.75 | 0.5953 | 632.0 | 526.6 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -11.07 | 161.10 | 29.15 | 238.91 | 0.5604 | -366.0 | -305.6 | |
| 0.00 | 1.49 | 0.00 | 0.89 | -11.05 | 160.78 | 28.83 | 238.66 | 0.5564 | -702.0 | -500.5 | |
| 0.44 | 1.93 | 0.26 | 1.13 | -10.68 | 158.77 | 26.83 | 237.36 | 0.5287 | -830.4 | -662.2 | |
| 0.00 | 2.37 | 0.00 | 1.41 | -14.28 | 158.62 | 26.68 | 231.69 | 0.5566 | -734.0 | -562.0 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -13.18 | 158.35 | 26.40 | 233.03 | 0.5441 | -551.0 | -520.6 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -11.59 | 158.11 | 26.16 | 235.24 | 0.5278 | -717.0 | -560.1 | |
| 2.55 | 8.79 | 1.50 | 5.19 | -13.55 | 158.12 | 26.17 | 232.23 | 0.5445 | -771.4 | -545.8 | |
| 0.00 | 0.70 | 0.00 | 0.41 | -12.43 | 157.38 | 25.43 | 233.14 | 0.5262 | -642.0 | -567.4 | |
| 8.09 | 16.26 | 4.73 | 9.52 | -13.20 | 157.42 | 25.48 | 232.02 | 0.5334 | -963.3 | -726.2 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -19.82 | 146.08 | 14.13 | 207.53 | 0.4990 | -655.0 | -508.2 | |
| 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. | |