SOHO MDI 2001-02-05 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39 | 330 | 22 | 191 | 24.22 | 113.89 | 3.71 | 353.34 | 0.5109 | 1159.3 | 287.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2001-02-05 11:11:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30 | 179 | 17 | 103 | 23.22 | 116.93 | 6.75 | 347.62 | 0.5056 | 1526.8 | 590.9 | |
| 0 | 18 | 0 | 10 | 20.90 | 112.21 | 2.02 | 355.88 | 0.4601 | 677.0 | 677.2 | |
| 0 | 3 | 0 | 2 | 24.50 | 111.50 | 1.32 | 357.66 | 0.5145 | 731.0 | 666.3 | |
| 7 | 48 | 4 | 28 | 25.09 | 111.38 | 1.19 | 357.92 | 0.5231 | 861.7 | 159.1 | |
| 0 | 4 | 0 | 2 | 21.85 | 111.35 | 1.17 | 357.71 | 0.4741 | 598.0 | 427.5 | |
| 0 | 8 | 0 | 5 | 24.41 | 111.04 | 0.85 | 358.48 | 0.5129 | 717.0 | 810.3 | |
| 0 | 6 | 0 | 3 | 26.77 | 110.93 | 0.74 | 358.79 | 0.5478 | -498.0 | -385.8 | |
| 2 | 12 | 1 | 7 | 26.35 | 110.63 | 0.44 | 359.27 | 0.5416 | -819.1 | -588.3 | |
| 0 | 5 | 0 | 3 | 19.36 | 110.32 | 0.13 | 359.72 | 0.4347 | 766.0 | 573.7 | |
| 0 | 5 | 0 | 3 | 27.04 | 109.72 | -0.47 | 0.75 | 0.5517 | -837.0 | -770.8 | |
| 0 | 3 | 0 | 2 | 29.52 | 108.79 | -1.40 | 2.09 | 0.5877 | -471.0 | -363.7 | |
| 0 | 7 | 0 | 4 | 27.55 | 108.25 | -1.94 | 3.08 | 0.5599 | -863.0 | -611.7 | |
| 0 | 17 | 0 | 10 | 27.05 | 108.17 | -2.02 | 3.27 | 0.5526 | -837.0 | -803.0 | |
| 0 | 11 | 0 | 6 | 29.19 | 107.87 | -2.32 | 3.49 | 0.5837 | -911.0 | -837.5 | |
| 0 | 4 | 0 | 3 | 29.67 | 106.88 | -3.31 | 4.88 | 0.5915 | -551.0 | -460.3 | |
| 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. | |