SOHO MDI 2000-11-27 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 150 | 952 | 127 | 805 | 19.66 | 358.32 | 52.01 | 293.63 | 0.8122 | 743.2 | 419.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-27 22:23:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 864 | 5 | 733 | 18.78 | 359.21 | 52.90 | 292.34 | 0.8186 | 1016.9 | 433.0 | |
| 47 | -1 | 41 | -1 | 20.36 | 359.62 | 53.31 | 294.11 | 0.8258 | 467.1 | 999999 | |
| 10 | -1 | 9 | -1 | 18.55 | 358.37 | 52.06 | 292.27 | 0.8102 | 1019.6 | 999999 | |
| 28 | -1 | 24 | -1 | 19.88 | 358.64 | 52.33 | 293.80 | 0.8158 | 1202.2 | 999999 | |
| 6 | -1 | 5 | -1 | 17.40 | 357.50 | 51.19 | 291.09 | 0.7993 | -707.3 | 999999 | |
| 14 | -1 | 12 | -1 | 20.37 | 358.74 | 52.43 | 294.36 | 0.8179 | 1240.9 | 999999 | |
| 5 | -1 | 4 | -1 | 17.96 | 357.53 | 51.22 | 291.77 | 0.8008 | 81.3 | 999999 | |
| 0 | 4 | 0 | 4 | 16.29 | 356.89 | 50.59 | 289.87 | 0.7908 | -288.0 | -209.2 | |
| -4 | -1 | -4 | -1 | 19.81 | 358.07 | 51.76 | 293.87 | 0.8103 | 999999 | 999999 | |
| 19 | -1 | 15 | -1 | 18.17 | 357.10 | 50.79 | 292.14 | 0.7971 | 804.4 | 999999 | |
| 6 | -1 | 5 | -1 | 19.10 | 356.53 | 50.22 | 293.44 | 0.7938 | 949.2 | 999999 | |
| 0 | 10 | 0 | 8 | 21.29 | 357.19 | 50.88 | 295.91 | 0.8059 | 148.0 | 160.8 | |
| 3 | 46 | 2 | 37 | 20.90 | 356.04 | 49.73 | 295.79 | 0.7939 | 490.8 | 354.9 | |
| 0 | 5 | 0 | 4 | 22.37 | 356.74 | 50.43 | 297.34 | 0.8047 | 172.0 | 84.2 | |
| 6 | 18 | 5 | 15 | 21.80 | 356.14 | 49.83 | 296.85 | 0.7975 | 670.7 | 578.8 | |
| 0 | 5 | 0 | 4 | 22.56 | 348.38 | 42.07 | 300.85 | 0.7232 | -601.0 | -637.9 | |
| 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. | |