SOHO MDI 2000-11-08 00:13:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61 | 353 | 38 | 217 | -12.22 | 176.31 | -32.49 | 116.63 | 0.5894 | 575.1 | 297.7 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-08 00:13:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -13.80 | 179.36 | -29.44 | 121.32 | 0.5609 | -607.0 | -518.0 | |
| 0 | 6 | 0 | 4 | -12.06 | 178.77 | -30.03 | 118.07 | 0.5568 | 952.0 | 762.8 | |
| 9 | 246 | 6 | 149 | -13.58 | 177.74 | -31.06 | 119.68 | 0.5794 | 1153.3 | 611.1 | |
| 12 | -3 | 7 | -3 | -12.45 | 177.71 | -31.08 | 117.91 | 0.5727 | 1653.0 | 999999 | |
| 8 | -3 | 5 | -3 | -12.39 | 177.40 | -31.40 | 117.57 | 0.5763 | 1313.2 | 999999 | |
| 7 | -3 | 4 | -3 | -12.60 | 176.95 | -31.84 | 117.59 | 0.5832 | 1113.0 | 999999 | |
| 7 | -3 | 4 | -3 | -13.05 | 176.79 | -32.00 | 118.16 | 0.5878 | 951.8 | 999999 | |
| 2 | -3 | 1 | -3 | -12.37 | 176.75 | -32.04 | 117.08 | 0.5843 | 1083.9 | 999999 | |
| 0 | 6 | 0 | 4 | -12.04 | 175.86 | -32.93 | 115.97 | 0.5937 | 689.0 | 567.2 | |
| 0 | 21 | 0 | 13 | -10.58 | 174.31 | -34.49 | 112.76 | 0.6058 | -944.0 | -611.7 | |
| 12 | 61 | 8 | 39 | -10.62 | 173.30 | -35.49 | 112.25 | 0.6189 | -1162.8 | -523.7 | |
| 0 | 4 | 0 | 3 | -11.42 | 173.04 | -35.75 | 113.32 | 0.6260 | -362.0 | -293.9 | |
| 4 | -11 | 3 | -11 | -10.80 | 172.69 | -36.10 | 112.20 | 0.6274 | -793.7 | 999999 | |
| 0 | 5 | 0 | 3 | -11.00 | 171.79 | -37.01 | 112.01 | 0.6397 | -600.0 | -496.1 | |
| 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. | |