| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9 | 116 | 6 | 73 | -27.62 | 290.91 | 22.26 | 212.83 | 0.6215 | 658.0 | 471.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-03 11:11:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -27.42 | 293.44 | 24.78 | 215.79 | 0.6386 | 524.0 | 484.1 | |
| 0 | 5 | 0 | 3 | -27.63 | 293.06 | 24.40 | 215.17 | 0.6378 | 471.0 | 482.9 | |
| 0 | 3 | 0 | 2 | -27.20 | 292.34 | 23.69 | 214.83 | 0.6278 | 592.0 | 617.6 | |
| 0 | 6 | 0 | 3 | -26.48 | 292.13 | 23.48 | 215.35 | 0.6186 | 741.0 | 676.4 | |
| 0 | 7 | 0 | 5 | -26.11 | 291.68 | 23.02 | 215.23 | 0.6111 | 942.0 | 818.6 | |
| 0 | 3 | 0 | 2 | -26.78 | 291.68 | 23.03 | 214.54 | 0.6182 | 745.0 | 706.3 | |
| 0 | 6 | 0 | 3 | -27.00 | 291.40 | 22.74 | 214.00 | 0.6183 | 971.0 | 863.3 | |
| 0 | 11 | 0 | 7 | -26.63 | 291.04 | 22.39 | 213.97 | 0.6116 | 782.0 | 794.2 | |
| 0 | 6 | 0 | 4 | -28.76 | 291.37 | 22.71 | 212.23 | 0.6370 | 428.0 | 386.4 | |
| 0 | 8 | 0 | 5 | -27.39 | 291.01 | 22.36 | 213.17 | 0.6197 | 669.0 | 570.4 | |
| 9 | 20 | 6 | 13 | -28.11 | 290.94 | 22.28 | 212.37 | 0.6269 | 714.2 | 354.1 | |
| 0 | 6 | 0 | 4 | -28.05 | 290.26 | 21.61 | 211.67 | 0.6213 | 439.0 | 157.8 | |
| 0 | 4 | 0 | 3 | -29.88 | 290.29 | 21.63 | 210.00 | 0.6417 | -277.0 | -164.9 | |
| 0 | 7 | 0 | 4 | -26.99 | 289.49 | 20.83 | 211.79 | 0.6039 | 1051.0 | 822.4 | |
| 0 | 10 | 0 | 6 | -28.03 | 289.60 | 20.95 | 210.92 | 0.6164 | 599.0 | 479.8 | |
| 0 | 7 | 0 | 4 | -29.41 | 289.75 | 21.10 | 209.83 | 0.6328 | -698.0 | -665.4 | |
| 0 | 4 | 0 | 3 | -26.62 | 288.96 | 20.30 | 211.51 | 0.5957 | 862.0 | 806.6 | |
| 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. | |