| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.04 | 145.47 | 19.66 | 78.88 | 6.06 | 204.32 | 23.64 | 276.26 | 0.4026 | -210.1 | -91.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-11 14:00:40 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 | 3.27 | 0.00 | 1.80 | 4.40 | 206.40 | 25.71 | 271.92 | 0.4346 | -802.0 | -533.3 | |
| 17.07 | 72.55 | 9.37 | 39.87 | 5.84 | 206.26 | 25.57 | 275.25 | 0.4330 | -1043.9 | -325.7 | |
| 0.00 | 2.00 | 0.00 | 1.09 | 5.30 | 205.96 | 25.28 | 274.03 | 0.4280 | -776.0 | -607.0 | |
| 0.00 | 3.09 | 0.00 | 1.69 | 3.77 | 205.90 | 25.22 | 270.45 | 0.4269 | -571.0 | -510.6 | |
| 5.63 | -2.00 | 3.08 | -2.00 | 5.82 | 205.78 | 25.10 | 275.28 | 0.4256 | -1183.0 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 10.46 | 206.07 | 25.39 | 285.87 | 0.4401 | -676.0 | -612.9 | |
| 2.63 | 4.27 | 1.44 | 2.33 | 4.28 | 205.48 | 24.80 | 271.62 | 0.4201 | -889.7 | -664.7 | |
| 0.00 | 2.45 | 0.00 | 1.34 | 3.37 | 205.25 | 24.57 | 269.43 | 0.4168 | -968.0 | -823.0 | |
| 0.00 | 2.00 | 0.00 | 1.09 | 4.86 | 205.30 | 24.62 | 273.03 | 0.4174 | -976.0 | -804.1 | |
| 0.91 | 2.81 | 0.49 | 1.52 | 6.21 | 204.15 | 23.47 | 276.46 | 0.4001 | -980.2 | -879.0 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 8.07 | 204.26 | 23.57 | 281.05 | 0.4051 | 129.0 | 218.9 | |
| 0.00 | 0.64 | 0.00 | 0.34 | 7.43 | 204.12 | 23.43 | 279.52 | 0.4015 | -710.0 | -511.7 | |
| 3.63 | 5.63 | 1.97 | 3.05 | 8.37 | 204.14 | 23.46 | 281.85 | 0.4041 | 910.8 | 667.5 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 8.07 | 204.02 | 23.34 | 281.15 | 0.4015 | 222.0 | 233.5 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 7.95 | 203.98 | 23.30 | 280.86 | 0.4005 | 630.0 | 386.0 | |
| 2.18 | 4.27 | 1.17 | 2.30 | 6.15 | 203.78 | 23.10 | 276.41 | 0.3942 | -978.9 | -635.3 | |
| 2.45 | 4.99 | 1.32 | 2.69 | 8.12 | 203.46 | 22.77 | 281.48 | 0.3927 | 1106.5 | 853.5 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 7.94 | 203.44 | 22.76 | 281.02 | 0.3920 | 832.0 | 636.2 | |
| 1.18 | 3.72 | 0.63 | 2.00 | 6.30 | 203.09 | 22.41 | 276.91 | 0.3833 | -940.1 | -513.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 6.51 | 202.93 | 22.25 | 277.52 | 0.3811 | -799.0 | -695.7 | |
| 0.36 | 3.36 | 0.19 | 1.79 | 7.08 | 202.40 | 21.72 | 279.16 | 0.3735 | 982.5 | 741.7 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 4.85 | 202.27 | 21.59 | 273.19 | 0.3687 | 804.0 | 738.1 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 6.57 | 201.91 | 21.23 | 277.95 | 0.3648 | 895.0 | 795.3 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 6.00 | 201.76 | 21.07 | 276.40 | 0.3614 | 717.0 | 634.5 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 6.85 | 201.66 | 20.98 | 278.79 | 0.3613 | 776.0 | 599.5 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 5.94 | 201.59 | 20.91 | 276.28 | 0.3586 | 610.0 | 416.8 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 5.79 | 200.05 | 19.37 | 276.21 | 0.3333 | 837.0 | 603.1 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 5.96 | 199.57 | 18.89 | 276.83 | 0.3256 | 765.0 | 586.7 | |
| 0.00 | 3.27 | 0.00 | 1.69 | 6.58 | 197.66 | 16.97 | 279.53 | 0.2954 | 820.0 | 646.9 | |
| 0.00 | 2.00 | 0.00 | 1.04 | 6.31 | 197.62 | 16.93 | 278.62 | 0.2941 | 944.0 | 747.9 | |
| 0.00 | 7.72 | 0.00 | 3.97 | 6.52 | 196.12 | 15.44 | 280.10 | 0.2698 | 981.0 | 763.3 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 4.92 | 195.03 | 14.35 | 274.39 | 0.2487 | 834.0 | 737.5 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 5.58 | 192.25 | 11.57 | 278.45 | 0.2027 | -632.0 | -566.1 | |
| 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. | |