SOHO MDI 2000-11-02 09:56:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 110 | 794 | 56 | 399 | 2.65 | 272.00 | -10.52 | 98.00 | 0.1852 | 1837.4 | 698.9 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-02 09:56:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37 | 728 | 19 | 366 | 2.24 | 273.01 | -9.51 | 101.05 | 0.1690 | 2200.5 | 732.0 | |
| 0 | 5 | 0 | 2 | 4.36 | 272.79 | -9.72 | 88.40 | 0.1693 | -404.0 | -160.8 | |
| 21 | -1 | 11 | -1 | 2.16 | 272.46 | -10.06 | 100.89 | 0.1785 | 1772.2 | 999999 | |
| 13 | -1 | 7 | -1 | 3.35 | 272.22 | -10.30 | 94.09 | 0.1798 | 1631.8 | 999999 | |
| 0 | 2 | 0 | 1 | 4.19 | 271.97 | -10.55 | 89.37 | 0.1834 | 526.0 | 537.3 | |
| 5 | -1 | 2 | -1 | 3.31 | 271.71 | -10.81 | 94.10 | 0.1886 | 1405.8 | 999999 | |
| 29 | -1 | 15 | -1 | 2.88 | 271.67 | -10.84 | 96.32 | 0.1899 | 1891.6 | 999999 | |
| 5 | -1 | 2 | -1 | 3.69 | 271.47 | -11.05 | 92.01 | 0.1923 | 1207.4 | 999999 | |
| 0 | 7 | 0 | 4 | 0.34 | 271.49 | -11.03 | 108.81 | 0.2030 | 803.0 | 597.1 | |
| 0 | 9 | 0 | 5 | 4.29 | 270.47 | -12.04 | 88.89 | 0.2091 | 609.0 | 369.5 | |
| 0 | 5 | 0 | 2 | 2.25 | 270.26 | -12.25 | 98.47 | 0.2154 | 121.0 | 109.8 | |
| 0 | 7 | 0 | 3 | 4.27 | 269.41 | -13.11 | 88.98 | 0.2273 | 892.0 | 681.0 | |
| 0 | 5 | 0 | 3 | 3.46 | 267.11 | -15.41 | 92.03 | 0.2665 | 756.0 | 695.8 | |
| 0 | 11 | 0 | 6 | 1.37 | 266.66 | -15.86 | 99.49 | 0.2783 | 778.0 | 786.7 | |
| 0 | 4 | 0 | 2 | 2.40 | 266.05 | -16.47 | 95.55 | 0.2859 | 628.0 | 556.1 | |
| 0 | 7 | 0 | 3 | 5.14 | 264.37 | -18.15 | 86.16 | 0.3123 | -992.0 | -840.5 | |
| 0 | 4 | 0 | 2 | 2.57 | 259.03 | -23.49 | 93.09 | 0.4005 | -678.0 | -577.8 | |
| 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. | |