SOHO MDI 2000-11-05 19:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 101 | 0 | 58 | 9.81 | 268.91 | 31.00 | 283.33 | 0.5225 | 134.4 | 276.0 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-05 19:11:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 7 | 0 | 5 | 6.64 | 276.16 | 38.25 | 275.93 | 0.6205 | 765.0 | 757.0 | |
| 0 | 5 | 0 | 3 | 7.26 | 276.17 | 38.26 | 276.93 | 0.6211 | 739.0 | 651.9 | |
| 0 | 5 | 0 | 3 | 10.69 | 273.55 | 35.64 | 283.02 | 0.5899 | 304.0 | 446.8 | |
| 0 | 4 | 0 | 2 | 10.39 | 273.22 | 35.31 | 282.59 | 0.5848 | 618.0 | 564.4 | |
| 0 | 7 | 0 | 4 | 9.39 | 272.05 | 34.14 | 281.12 | 0.5665 | 519.0 | 537.5 | |
| 0 | 7 | 0 | 4 | 10.07 | 271.47 | 33.56 | 282.46 | 0.5596 | 362.0 | 557.6 | |
| 0 | 11 | 0 | 6 | 8.98 | 269.50 | 31.59 | 280.95 | 0.5291 | 32.0 | 98.3 | |
| 0 | 4 | 0 | 2 | 10.29 | 269.59 | 31.68 | 283.38 | 0.5333 | 561.0 | 527.4 | |
| 0 | 14 | 0 | 8 | 9.60 | 269.38 | 31.47 | 282.15 | 0.5286 | 1163.0 | 903.8 | |
| 0 | 5 | 0 | 3 | 8.81 | 267.53 | 29.62 | 281.13 | 0.4999 | 574.0 | 379.8 | |
| 0 | 2 | 0 | 1 | 11.73 | 267.29 | 29.38 | 286.95 | 0.5043 | 266.0 | 441.8 | |
| 0 | 3 | 0 | 2 | 11.54 | 267.00 | 29.09 | 286.72 | 0.4995 | 657.0 | 534.2 | |
| 0 | 7 | 0 | 4 | 11.28 | 265.23 | 27.33 | 287.01 | 0.4727 | -686.0 | -518.0 | |
| 0 | 3 | 0 | 2 | 7.69 | 263.84 | 25.93 | 279.76 | 0.4416 | -541.0 | -351.3 | |
| 0 | 5 | 0 | 3 | 12.71 | 262.97 | 25.06 | 291.31 | 0.4454 | -582.0 | -472.3 | |
| 0 | 4 | 0 | 2 | 9.38 | 261.17 | 23.26 | 284.77 | 0.4048 | -658.0 | -583.0 | |
| 0 | 3 | 0 | 1 | 12.25 | 261.41 | 23.50 | 291.36 | 0.4203 | -815.0 | -790.9 | |
| 0 | 5 | 0 | 3 | 13.76 | 256.63 | 18.72 | 299.52 | 0.3599 | -859.0 | -652.5 | |
| 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. | |