SOHO MDI 2000-11-02 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 106 | 0 | 63 | -26.97 | 291.33 | 9.50 | 195.81 | 0.5391 | 769.7 | 764.9 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-02 11:11:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 2 | 0 | 1 | -30.50 | 295.87 | 14.04 | 200.25 | 0.6062 | 472.0 | 528.0 | |
| 0 | 9 | 0 | 6 | -28.77 | 294.86 | 13.03 | 200.04 | 0.5788 | 552.0 | 594.9 | |
| 0 | 13 | 0 | 8 | -26.71 | 293.95 | 12.12 | 200.14 | 0.5468 | 693.0 | 652.2 | |
| 0 | 4 | 0 | 2 | -28.57 | 294.07 | 12.24 | 199.06 | 0.5725 | 531.0 | 454.0 | |
| 0 | 8 | 0 | 4 | -25.60 | 291.79 | 9.96 | 197.48 | 0.5213 | 860.0 | 751.3 | |
| 0 | 5 | 0 | 3 | -26.41 | 291.86 | 10.03 | 197.09 | 0.5329 | 1040.0 | 894.8 | |
| 0 | 19 | 0 | 11 | -27.03 | 291.26 | 9.42 | 195.76 | 0.5391 | 1089.0 | 931.0 | |
| 0 | 11 | 0 | 7 | -27.01 | 289.90 | 8.07 | 193.60 | 0.5338 | 1085.0 | 955.0 | |
| 0 | 4 | 0 | 2 | -27.42 | 289.71 | 7.88 | 193.10 | 0.5389 | 957.0 | 841.3 | |
| 0 | 4 | 0 | 2 | -25.22 | 289.52 | 7.69 | 193.87 | 0.5066 | 894.0 | 799.6 | |
| 0 | 8 | 0 | 5 | -25.67 | 289.46 | 7.63 | 193.55 | 0.5128 | 889.0 | 710.8 | |
| 0 | 12 | 0 | 7 | -27.14 | 289.30 | 7.47 | 192.57 | 0.5336 | 1190.0 | 1000.7 | |
| 0 | 4 | 0 | 3 | -27.37 | 289.09 | 7.26 | 192.13 | 0.5362 | 889.0 | 771.1 | |
| 0 | 3 | 0 | 2 | -25.74 | 287.53 | 5.70 | 190.18 | 0.5079 | -365.0 | -401.4 | |
| 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. | |