SOHO MDI 2000-11-03 04:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82 | 469 | 55 | 316 | -23.23 | 305.22 | 33.05 | 228.18 | 0.6746 | -778.1 | -358.1 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-03 04:47:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 3 | -19.53 | 306.83 | 34.66 | 234.07 | 0.6643 | 273.0 | 283.4 | |
| 15 | 83 | 10 | 57 | -22.53 | 307.54 | 35.37 | 230.83 | 0.6921 | -1145.5 | -571.4 | |
| 13 | 264 | 9 | 179 | -24.06 | 306.01 | 33.84 | 227.84 | 0.6884 | -1043.3 | -346.9 | |
| 4 | -3 | 3 | -3 | -23.83 | 305.58 | 33.42 | 227.78 | 0.6826 | -1391.3 | 999999 | |
| 12 | -3 | 8 | -3 | -24.31 | 305.63 | 33.46 | 227.25 | 0.6866 | -871.7 | 999999 | |
| 9 | -3 | 6 | -3 | -23.55 | 305.10 | 32.93 | 227.73 | 0.6759 | -1214.2 | 999999 | |
| 2 | 7 | 1 | 5 | -23.12 | 304.29 | 32.12 | 227.57 | 0.6648 | -787.8 | -767.2 | |
| 14 | 51 | 9 | 33 | -20.41 | 303.56 | 31.39 | 230.35 | 0.6364 | -1012.2 | -637.6 | |
| 3 | -3 | 2 | -3 | -25.19 | 304.73 | 32.56 | 225.50 | 0.6852 | -211.1 | 999999 | |
| 0 | 6 | 0 | 4 | -22.68 | 303.92 | 31.75 | 227.80 | 0.6578 | -957.0 | -916.4 | |
| 0 | 7 | 0 | 5 | -22.79 | 303.56 | 31.39 | 227.36 | 0.6552 | -1212.0 | -1033.1 | |
| 0 | 8 | 0 | 5 | -22.95 | 303.06 | 30.89 | 226.74 | 0.6516 | -320.0 | -296.3 | |
| 2 | 8 | 2 | 6 | -25.57 | 303.28 | 31.11 | 223.85 | 0.6753 | 805.6 | 630.7 | |
| 8 | 31 | 5 | 19 | -22.40 | 299.77 | 27.60 | 224.35 | 0.6151 | 1001.8 | 635.0 | |
| 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. | |