| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61 | 467 | 38 | 286 | -8.94 | 324.65 | 32.67 | 244.74 | 0.5904 | -1444.6 | -444.9 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-10-05 09:17:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56 | 377 | 35 | 235 | -9.03 | 326.33 | 34.35 | 246.04 | 0.6121 | -1604.3 | -549.0 | |
| -1 | -1 | -1 | -1 | -8.96 | 325.80 | 33.82 | 245.81 | 0.6050 | 999999 | 999999 | |
| 5 | 11 | 3 | 6 | -8.12 | 323.98 | 32.01 | 245.90 | 0.5770 | -810.8 | -567.6 | |
| 0 | 7 | 0 | 4 | -6.84 | 323.87 | 31.90 | 247.90 | 0.5685 | 572.0 | 364.9 | |
| 0 | 6 | 0 | 4 | -8.60 | 323.88 | 31.91 | 245.07 | 0.5786 | -888.0 | -679.9 | |
| 0 | 5 | 0 | 3 | -8.33 | 322.07 | 30.10 | 244.17 | 0.5534 | -647.0 | -579.7 | |
| 0 | 8 | 0 | 5 | -9.35 | 320.89 | 28.92 | 241.56 | 0.5448 | -717.0 | -616.2 | |
| 0 | 5 | 0 | 3 | -8.61 | 320.69 | 28.72 | 242.60 | 0.5373 | -450.0 | -420.1 | |
| 0 | 7 | 0 | 4 | -4.61 | 320.40 | 28.42 | 249.39 | 0.5089 | -893.0 | -729.8 | |
| 0 | 3 | 0 | 2 | -9.36 | 316.44 | 24.47 | 237.29 | 0.4877 | 542.0 | 651.1 | |
| 0 | 4 | 0 | 2 | -7.79 | 315.69 | 23.72 | 239.29 | 0.4654 | 641.0 | 629.9 | |
| 0 | 6 | 0 | 3 | -8.24 | 314.99 | 23.02 | 237.68 | 0.4598 | 1001.0 | 996.9 | |
| 0 | 18 | 0 | 10 | -10.74 | 311.14 | 19.17 | 228.08 | 0.4353 | 707.0 | 681.1 | |
| 0 | 6 | 0 | 3 | -9.93 | 310.92 | 18.95 | 229.21 | 0.4243 | 851.0 | 672.4 | |
| 0 | 4 | 0 | 2 | -10.40 | 310.61 | 18.64 | 227.90 | 0.4256 | 389.0 | 535.2 | |
| 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. | |