SOHO MDI 2000-11-01 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 104 | 732 | 56 | 393 | 2.62 | 271.61 | -22.52 | 93.45 | 0.3848 | 1665.0 | 623.6 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-01 12:47:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32 | 682 | 17 | 364 | 2.26 | 272.90 | -21.23 | 94.67 | 0.3646 | 2145.4 | 662.7 | |
| 0 | 4 | 0 | 2 | 0.13 | 272.46 | -21.66 | 100.21 | 0.3768 | -353.0 | -226.2 | |
| 15 | -1 | 8 | -1 | 2.13 | 272.41 | -21.72 | 94.88 | 0.3728 | 1538.9 | 999999 | |
| 13 | -1 | 7 | -1 | 3.39 | 271.93 | -22.20 | 91.43 | 0.3790 | 1625.3 | 999999 | |
| 0 | 9 | 0 | 5 | 0.96 | 271.92 | -22.21 | 97.79 | 0.3831 | 796.0 | 585.9 | |
| 6 | -1 | 3 | -1 | 2.30 | 271.61 | -22.52 | 94.22 | 0.3853 | 1230.6 | 999999 | |
| 35 | -1 | 19 | -1 | 2.87 | 271.44 | -22.69 | 92.69 | 0.3874 | 1590.8 | 999999 | |
| 3 | -1 | 2 | -1 | 2.78 | 270.94 | -23.19 | 92.83 | 0.3956 | 854.5 | 999999 | |
| 0 | 6 | 0 | 3 | 4.69 | 270.17 | -23.96 | 88.00 | 0.4068 | 762.0 | 627.4 | |
| 0 | 3 | 0 | 2 | 4.83 | 269.74 | -24.39 | 87.66 | 0.4137 | 299.0 | 249.8 | |
| 0 | 3 | 0 | 2 | 0.52 | 266.44 | -27.69 | 96.92 | 0.4701 | 815.0 | 753.2 | |
| 0 | 3 | 0 | 2 | 2.18 | 265.37 | -28.76 | 93.20 | 0.4836 | 496.0 | 450.1 | |
| 0 | 6 | 0 | 3 | 1.49 | 263.56 | -30.57 | 94.23 | 0.5119 | 680.0 | 527.2 | |
| 0 | 4 | 0 | 3 | 2.75 | 260.24 | -33.89 | 91.38 | 0.5593 | -478.0 | -488.4 | |
| 0 | 12 | 0 | 7 | 4.89 | 259.77 | -34.36 | 87.53 | 0.5650 | -758.0 | -503.0 | |
| 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. | |