SOHO MDI 2000-01-26 10:27:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 124 | 699 | 80 | 453 | 5.07 | 71.78 | 38.59 | 284.85 | 0.6445 | -207.8 | -92.7 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-01-26 10:27:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32 | 295 | 22 | 199 | 3.86 | 75.46 | 42.27 | 281.62 | 0.6876 | 1359.7 | 503.4 | |
| 9 | -1 | 6 | -1 | 4.44 | 75.44 | 42.26 | 282.46 | 0.6890 | 801.5 | 999999 | |
| -1 | -1 | -1 | -1 | 3.45 | 75.12 | 41.94 | 281.14 | 0.6823 | 999999 | 999999 | |
| 0 | 7 | 0 | 5 | 4.96 | 75.07 | 41.88 | 283.32 | 0.6859 | 627.0 | 475.0 | |
| 6 | -1 | 4 | -1 | 4.44 | 74.77 | 41.59 | 282.67 | 0.6806 | 1136.2 | 999999 | |
| 6 | -1 | 4 | -1 | 4.82 | 74.08 | 40.89 | 283.46 | 0.6732 | 940.6 | 999999 | |
| 4 | -1 | 2 | -1 | 4.77 | 73.26 | 40.08 | 283.67 | 0.6627 | 836.8 | 999999 | |
| 0 | 5 | 0 | 4 | 3.53 | 72.74 | 39.55 | 282.02 | 0.6522 | 772.0 | 835.5 | |
| 0 | 11 | 0 | 7 | 3.54 | 72.24 | 39.06 | 282.21 | 0.6458 | 441.0 | 513.6 | |
| 3 | 8 | 2 | 5 | 4.97 | 72.08 | 38.89 | 284.41 | 0.6482 | 900.7 | 709.6 | |
| 0 | 14 | 0 | 9 | 4.03 | 70.70 | 37.51 | 283.52 | 0.6271 | -415.0 | -386.7 | |
| 0 | 5 | 0 | 3 | 6.80 | 70.17 | 36.99 | 288.01 | 0.6305 | -608.0 | -557.8 | |
| 5 | 354 | 3 | 221 | 6.75 | 69.20 | 36.02 | 288.39 | 0.6177 | -758.0 | -678.2 | |
| 32 | -13 | 20 | -13 | 5.45 | 69.05 | 35.87 | 286.44 | 0.6105 | -1664.5 | 999999 | |
| 6 | -13 | 4 | -13 | 6.54 | 68.95 | 35.76 | 288.20 | 0.6135 | -1241.8 | 999999 | |
| -14 | -13 | -14 | -13 | 5.75 | 68.79 | 35.61 | 287.03 | 0.6082 | 999999 | 999999 | |
| 21 | -13 | 13 | -13 | 6.59 | 68.48 | 35.29 | 288.51 | 0.6076 | -1766.6 | 999999 | |
| 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. | |