| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.54 | 298.00 | 59.70 | 430.50 | -22.95 | 107.29 | 68.44 | 245.62 | 0.9416 | 521.5 | 260.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-10 15:58:55 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 |
| 2.04 | 264.01 | 3.19 | 386.08 | -23.24 | 108.82 | 69.97 | 245.53 | 0.9500 | -215.2 | 273.5 | |
| 0.00 | 13.63 | 0.00 | 18.78 | -21.17 | 106.28 | 67.43 | 247.35 | 0.9346 | 576.0 | 467.7 | |
| 37.73 | -1.00 | 55.50 | -1.00 | -23.05 | 107.50 | 68.65 | 245.54 | 0.9430 | 663.7 | 999999 | |
| 0.00 | 0.94 | 0.00 | 1.18 | -21.36 | 103.98 | 65.13 | 246.79 | 0.9211 | -65.0 | -34.2 | |
| 0.00 | 1.11 | 0.00 | 1.41 | -21.84 | 104.24 | 65.39 | 246.32 | 0.9232 | 309.0 | 287.6 | |
| 0.00 | 2.13 | 0.00 | 2.53 | -20.26 | 102.65 | 63.80 | 247.76 | 0.9112 | -535.0 | -417.2 | |
| 0.00 | 1.36 | 0.00 | 1.51 | -17.92 | 100.98 | 62.13 | 250.04 | 0.8968 | -558.0 | -399.7 | |
| 0.00 | 1.02 | 0.00 | 1.18 | -19.92 | 101.90 | 63.05 | 248.01 | 0.9057 | -372.0 | -306.7 | |
| 0.77 | 12.69 | 1.01 | 16.72 | -23.80 | 104.67 | 65.82 | 244.31 | 0.9279 | -300.3 | 21.1 | |
| 0.00 | 1.11 | 0.00 | 1.11 | -20.15 | 97.20 | 58.35 | 246.83 | 0.8713 | -418.0 | -319.2 | |
| 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. | |