SOHO MDI 2000-11-04 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44 | 281 | 47 | 294 | -23.59 | 305.18 | 56.73 | 240.50 | 0.8818 | -545.0 | -189.0 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-04 23:59:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 33 | 9 | 36 | -22.59 | 307.80 | 59.35 | 242.41 | 0.8981 | -560.1 | -271.0 | |
| 3 | 11 | 3 | 12 | -20.51 | 306.13 | 57.68 | 244.15 | 0.8814 | -378.1 | -299.3 | |
| 0 | 1 | 0 | 1 | -20.25 | 305.37 | 56.92 | 244.20 | 0.8751 | -424.0 | -353.1 | |
| 0 | 3 | 0 | 3 | -20.18 | 304.80 | 56.35 | 244.10 | 0.8706 | -583.0 | -578.5 | |
| 6 | 179 | 7 | 191 | -24.26 | 306.40 | 57.95 | 240.20 | 0.8924 | -198.6 | -185.2 | |
| 0 | 1 | 0 | 1 | -22.99 | 305.29 | 56.84 | 241.19 | 0.8814 | -356.0 | -356.0 | |
| 13 | -5 | 14 | -5 | -24.26 | 305.60 | 57.15 | 239.94 | 0.8869 | -775.7 | 999999 | |
| 0 | 8 | 0 | 8 | -20.45 | 302.98 | 54.53 | 243.21 | 0.8570 | -780.0 | -620.5 | |
| 0 | 8 | 0 | 8 | -23.42 | 304.58 | 56.13 | 240.49 | 0.8774 | -442.0 | -392.1 | |
| 14 | -5 | 14 | -5 | -24.71 | 305.22 | 56.77 | 239.33 | 0.8855 | -569.6 | 999999 | |
| 0 | 4 | 0 | 4 | -20.73 | 302.77 | 54.32 | 242.82 | 0.8561 | -550.0 | -491.9 | |
| 0 | 6 | 0 | 6 | -20.45 | 302.20 | 53.75 | 242.94 | 0.8506 | -451.0 | -491.6 | |
| 0 | 5 | 0 | 4 | -21.90 | 300.27 | 51.82 | 240.61 | 0.8393 | 314.0 | 250.2 | |
| 0 | 4 | 0 | 4 | -22.79 | 300.26 | 51.81 | 239.61 | 0.8422 | 253.0 | 237.3 | |
| 0 | 8 | 0 | 7 | -22.67 | 299.73 | 51.28 | 239.53 | 0.8375 | 408.0 | 384.6 | |
| 0 | 10 | 0 | 9 | -23.52 | 298.71 | 50.26 | 238.17 | 0.8321 | 537.0 | 441.0 | |
| 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. | |