| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.71 | 121.44 | 31.42 | 110.32 | 7.42 | 134.25 | 56.42 | 278.90 | 0.8355 | -124.4 | -26.0 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-07 16:58:56 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 |
| 11.85 | 68.09 | 11.63 | 67.17 | 7.24 | 137.31 | 59.48 | 278.33 | 0.8657 | -647.4 | -61.8 | |
| 8.69 | 10.65 | 8.32 | 10.19 | 7.15 | 136.41 | 58.59 | 278.31 | 0.8578 | -692.2 | -519.3 | |
| 0.00 | 1.45 | 0.00 | 1.35 | 5.90 | 135.67 | 57.84 | 276.90 | 0.8504 | -319.0 | -320.8 | |
| 0.00 | 1.11 | 0.00 | 1.00 | 6.88 | 134.35 | 56.52 | 278.18 | 0.8387 | -459.0 | -361.3 | |
| 0.00 | 1.02 | 0.00 | 0.92 | 6.65 | 134.09 | 56.26 | 277.92 | 0.8361 | -334.0 | -362.1 | |
| 0.00 | 0.94 | 0.00 | 0.78 | 6.65 | 131.28 | 53.45 | 278.19 | 0.8084 | -581.0 | -439.5 | |
| 0.00 | 0.85 | 0.00 | 0.66 | 10.57 | 127.44 | 49.62 | 283.69 | 0.7730 | 570.0 | 498.0 | |
| 15.17 | 35.88 | 11.47 | 27.19 | 8.05 | 126.41 | 48.58 | 280.60 | 0.7578 | 755.5 | 195.6 | |
| 0.00 | 1.11 | 0.00 | 0.82 | 6.09 | 125.87 | 48.04 | 278.08 | 0.7492 | 464.0 | 340.2 | |
| 0.00 | 0.34 | 0.00 | 0.24 | 7.94 | 122.77 | 44.94 | 281.07 | 0.7152 | 503.0 | 588.8 | |
| 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. | |