| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.42 | 163.16 | 18.28 | 117.21 | 17.41 | 62.08 | -43.76 | 65.89 | 0.7256 | -874.1 | -252.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-05 13:58:56 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 | 1.54 | 0.00 | 0.98 | 18.93 | 70.55 | -35.29 | 59.68 | 0.6354 | -818.0 | -717.1 | |
| 0.00 | 1.11 | 0.00 | 0.74 | 22.27 | 68.96 | -36.87 | 56.02 | 0.6720 | -636.0 | -525.3 | |
| 0.00 | 0.85 | 0.00 | 0.56 | 21.44 | 69.09 | -36.74 | 57.05 | 0.6659 | -640.0 | -529.6 | |
| 0.00 | 1.02 | 0.00 | 0.73 | 26.04 | 66.21 | -39.62 | 52.81 | 0.7216 | -510.0 | -401.9 | |
| 0.00 | 1.36 | 0.00 | 0.97 | 25.65 | 66.33 | -39.51 | 53.23 | 0.7183 | -640.0 | -505.0 | |
| 0.00 | 0.94 | 0.00 | 0.63 | 21.02 | 67.46 | -38.38 | 58.57 | 0.6816 | -558.0 | -418.5 | |
| 0.00 | 1.62 | 0.00 | 1.17 | 25.16 | 64.64 | -41.20 | 54.78 | 0.7321 | -486.0 | -436.5 | |
| 0.00 | 1.28 | 0.00 | 0.92 | 24.96 | 64.72 | -41.12 | 54.98 | 0.7304 | -643.0 | -481.0 | |
| 0.00 | 1.54 | 0.00 | 1.04 | 18.42 | 66.11 | -39.73 | 62.82 | 0.6840 | -623.0 | -504.8 | |
| 25.42 | 151.90 | 18.28 | 109.47 | 17.04 | 61.74 | -44.10 | 66.54 | 0.7277 | -1000.6 | -230.6 | |
| 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. | |