SOHO MDI 2000-11-11 07:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53 | 427 | 28 | 225 | -12.68 | 176.81 | 11.81 | 216.18 | 0.3396 | 1474.7 | 487.4 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-11 07:59:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 13 | 0 | 7 | -12.87 | 179.44 | 14.43 | 221.49 | 0.3684 | -973.0 | -753.3 | |
| 0 | 5 | 0 | 3 | -16.14 | 179.66 | 14.65 | 216.45 | 0.4108 | -666.0 | -522.2 | |
| 0 | 8 | 0 | 4 | -12.54 | 178.73 | 13.72 | 220.69 | 0.3568 | -524.0 | -276.7 | |
| 7 | 338 | 4 | 178 | -13.25 | 177.55 | 12.55 | 216.92 | 0.3536 | 1282.9 | 701.6 | |
| 15 | -4 | 8 | -4 | -12.17 | 177.38 | 12.37 | 218.50 | 0.3380 | 1930.8 | 999999 | |
| 14 | -4 | 7 | -4 | -12.84 | 177.13 | 12.12 | 216.70 | 0.3442 | 1481.2 | 999999 | |
| 17 | -4 | 9 | -4 | -12.60 | 176.79 | 11.79 | 216.38 | 0.3377 | 1779.8 | 999999 | |
| -7 | -4 | -7 | -4 | -12.84 | 176.69 | 11.68 | 215.70 | 0.3398 | 999999 | 999999 | |
| 0 | 4 | 0 | 2 | -13.63 | 175.92 | 10.91 | 212.56 | 0.3434 | 595.0 | 552.4 | |
| 0 | 18 | 0 | 9 | -13.43 | 175.51 | 10.50 | 211.91 | 0.3369 | 785.0 | 669.9 | |
| 0 | 4 | 0 | 2 | -9.89 | 175.25 | 10.25 | 217.91 | 0.2866 | -659.0 | -534.4 | |
| 0 | 7 | 0 | 4 | -8.62 | 174.74 | 9.74 | 219.39 | 0.2647 | -953.0 | -813.7 | |
| 0 | 3 | 0 | 2 | -9.64 | 174.22 | 9.21 | 215.53 | 0.2729 | -804.0 | -699.2 | |
| 0 | 6 | 0 | 3 | -15.63 | 173.83 | 8.83 | 204.68 | 0.3555 | -597.0 | -494.2 | |
| 0 | 4 | 0 | 2 | -15.10 | 173.61 | 8.60 | 204.78 | 0.3462 | -895.0 | -714.1 | |
| 0 | 5 | 0 | 3 | -13.28 | 173.02 | 8.02 | 205.64 | 0.3150 | -728.0 | -687.1 | |
| 0 | 4 | 0 | 2 | -12.96 | 172.49 | 7.49 | 204.60 | 0.3065 | -775.0 | -608.6 | |
| 0 | 4 | 0 | 2 | -10.80 | 171.02 | 6.01 | 203.10 | 0.2634 | -907.0 | -735.9 | |
| 0 | 4 | 0 | 2 | -12.14 | 169.51 | 4.50 | 196.21 | 0.2761 | -618.0 | -516.8 | |
| 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. | |