SOHO MDI 2000-11-07 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61 | 395 | 39 | 248 | -12.21 | 176.12 | -34.56 | 115.29 | 0.6155 | 453.9 | 259.4 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-07 20:47:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -13.78 | 179.26 | -31.42 | 119.74 | 0.5853 | -549.0 | -433.7 | |
| 0 | 5 | 0 | 3 | -12.19 | 178.70 | -31.98 | 116.87 | 0.5826 | 736.0 | 557.2 | |
| 9 | 273 | 6 | 169 | -13.59 | 177.65 | -33.03 | 118.29 | 0.6040 | 1116.3 | 586.7 | |
| 13 | -3 | 8 | -3 | -12.43 | 177.64 | -33.04 | 116.52 | 0.5974 | 1416.8 | 999999 | |
| -4 | -3 | -4 | -3 | -12.36 | 177.37 | -33.31 | 116.23 | 0.6004 | 999999 | 999999 | |
| 7 | -3 | 4 | -3 | -12.61 | 176.95 | -33.73 | 116.35 | 0.6070 | 1038.5 | 999999 | |
| 7 | -3 | 5 | -3 | -12.98 | 176.80 | -33.88 | 116.80 | 0.6109 | 920.6 | 999999 | |
| 2 | -3 | 1 | -3 | -12.38 | 176.75 | -33.93 | 115.87 | 0.6082 | 1004.2 | 999999 | |
| 6 | -3 | 4 | -3 | -12.85 | 176.05 | -34.63 | 116.13 | 0.6194 | 543.8 | 999999 | |
| 0 | 7 | 0 | 4 | -12.01 | 175.89 | -34.79 | 114.79 | 0.6169 | 487.0 | 482.2 | |
| 0 | 3 | 0 | 2 | -11.62 | 175.76 | -34.92 | 114.11 | 0.6166 | 600.0 | 448.8 | |
| 0 | 5 | 0 | 3 | -10.20 | 174.56 | -36.12 | 111.29 | 0.6250 | -684.0 | -640.9 | |
| 0 | 24 | 0 | 16 | -10.56 | 174.36 | -36.32 | 111.74 | 0.6291 | -1170.0 | -568.6 | |
| 0 | 5 | 0 | 4 | -9.91 | 173.87 | -36.81 | 110.51 | 0.6325 | -638.0 | -625.2 | |
| 5 | 62 | 4 | 40 | -10.48 | 173.44 | -37.23 | 111.15 | 0.6403 | -1142.4 | -566.0 | |
| 7 | -15 | 4 | -15 | -10.65 | 173.12 | -37.55 | 111.24 | 0.6450 | -1081.9 | 999999 | |
| 5 | -15 | 3 | -15 | -10.79 | 172.66 | -38.02 | 111.21 | 0.6514 | -759.8 | 999999 | |
| 0 | 6 | 0 | 4 | -10.98 | 171.67 | -39.01 | 111.03 | 0.6643 | -609.0 | -467.0 | |
| 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. | |