| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.08 | 73.14 | 24.48 | 83.69 | 7.39 | 135.68 | 63.91 | 278.26 | 0.8997 | -245.4 | 31.8 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-08 03:58:56 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 |
| 9.46 | 49.11 | 11.52 | 60.15 | 7.32 | 137.52 | 65.75 | 278.02 | 0.9150 | -557.6 | 1.6 | |
| 6.57 | 7.93 | 7.74 | 9.34 | 7.29 | 136.72 | 64.95 | 278.03 | 0.9093 | -536.2 | -397.0 | |
| 0.00 | 0.94 | 0.00 | 1.01 | 7.03 | 134.14 | 62.37 | 277.91 | 0.8897 | -358.0 | -294.0 | |
| 0.00 | 1.02 | 0.00 | 0.99 | 7.02 | 130.65 | 58.88 | 278.18 | 0.8605 | -536.0 | -449.8 | |
| 1.96 | 2.81 | 1.70 | 2.44 | 8.43 | 126.60 | 54.83 | 280.26 | 0.8240 | 381.7 | 333.9 | |
| 2.39 | 5.97 | 2.06 | 5.15 | 7.77 | 126.36 | 54.60 | 279.49 | 0.8210 | 441.2 | 491.8 | |
| 0.34 | -6.00 | 0.29 | -6.00 | 7.59 | 126.28 | 54.51 | 279.28 | 0.8200 | 721.2 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.18 | 8.31 | 126.37 | 54.60 | 280.14 | 0.8216 | 675.0 | 520.0 | |
| 1.36 | 2.81 | 1.17 | 2.42 | 8.04 | 126.26 | 54.49 | 279.83 | 0.8203 | 499.9 | 444.8 | |
| 0.00 | 1.19 | 0.00 | 1.01 | 6.58 | 125.69 | 53.92 | 278.10 | 0.8133 | 486.0 | 390.0 | |
| 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. | |