| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.81 | 136.93 | 17.01 | 97.41 | -24.31 | 283.03 | 38.85 | 232.80 | 0.7195 | 348.0 | 219.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-25 01:58:57 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 |
| 22.01 | 117.92 | 15.82 | 84.81 | -24.06 | 284.02 | 39.84 | 233.80 | 0.7273 | 975.6 | 324.8 | |
| 0.00 | 0.86 | 0.00 | 0.58 | -21.67 | 281.57 | 37.38 | 235.29 | 0.6887 | 753.0 | 597.6 | |
| 0.00 | 1.03 | 0.00 | 0.70 | -22.31 | 281.20 | 37.01 | 234.23 | 0.6888 | 577.0 | 501.1 | |
| 0.00 | 1.28 | 0.00 | 0.86 | -25.53 | 278.08 | 33.89 | 228.01 | 0.6793 | -693.0 | -484.9 | |
| 0.00 | 1.54 | 0.00 | 1.01 | -23.93 | 277.12 | 32.93 | 229.26 | 0.6582 | -683.0 | -620.7 | |
| 0.00 | 0.94 | 0.00 | 0.62 | -23.96 | 276.93 | 32.75 | 229.08 | 0.6565 | -793.0 | -609.6 | |
| 0.00 | 1.46 | 0.00 | 0.97 | -26.53 | 275.96 | 31.77 | 225.14 | 0.6670 | -682.0 | -638.5 | |
| 0.00 | 1.20 | 0.00 | 0.79 | -26.83 | 275.66 | 31.47 | 224.54 | 0.6666 | -630.0 | -566.0 | |
| 0.00 | 3.85 | 0.00 | 2.56 | -27.20 | 275.62 | 31.43 | 224.07 | 0.6693 | -616.0 | -451.8 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -26.52 | 275.26 | 31.07 | 224.57 | 0.6604 | -694.0 | -595.8 | |
| 1.80 | 2.65 | 1.19 | 1.75 | -26.88 | 275.17 | 30.99 | 224.06 | 0.6627 | -750.7 | -643.3 | |
| 0.00 | 2.31 | 0.00 | 1.52 | -27.11 | 274.74 | 30.55 | 223.42 | 0.6606 | -684.0 | -504.0 | |
| 0.00 | 0.86 | 0.00 | 0.56 | -27.68 | 274.37 | 30.19 | 222.44 | 0.6621 | -648.0 | -549.0 | |
| 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. | |