| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56 | 404 | 30 | 214 | -9.71 | 278.78 | 15.39 | 227.60 | 0.3566 | -1741.4 | -531.0 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-03 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 | -6.11 | 280.49 | 17.11 | 239.47 | 0.3411 | -711.0 | -580.1 | |
| 0 | 4 | 0 | 2 | -14.38 | 280.67 | 17.29 | 222.68 | 0.4265 | -528.0 | -538.6 | |
| 0 | 6 | 0 | 3 | -11.80 | 280.32 | 16.94 | 226.65 | 0.3939 | 542.0 | 351.6 | |
| 46 | 286 | 25 | 152 | -9.29 | 280.06 | 16.67 | 231.29 | 0.3644 | -1973.1 | -634.5 | |
| 10 | 49 | 5 | 26 | -9.78 | 278.74 | 15.36 | 227.92 | 0.3532 | -1509.6 | -891.2 | |
| 0 | 4 | 0 | 2 | -7.90 | 277.57 | 14.19 | 229.96 | 0.3186 | -879.0 | -735.3 | |
| 0 | 3 | 0 | 1 | -8.49 | 277.40 | 14.01 | 228.20 | 0.3227 | -614.0 | -717.6 | |
| 0 | 5 | 0 | 3 | -14.12 | 275.52 | 12.14 | 213.38 | 0.3722 | -946.0 | -775.3 | |
| 0 | 4 | 0 | 2 | -10.89 | 274.13 | 10.74 | 215.60 | 0.3159 | -423.0 | -368.5 | |
| 0 | 3 | 0 | 2 | -10.13 | 273.54 | 10.16 | 215.55 | 0.3000 | -581.0 | -402.6 | |
| 0 | 5 | 0 | 3 | -9.42 | 270.52 | 7.14 | 207.90 | 0.2632 | 549.0 | 457.2 | |
| 0 | 8 | 0 | 4 | -13.41 | 269.71 | 6.33 | 199.74 | 0.3188 | 905.0 | 789.5 | |
| 0 | 6 | 0 | 3 | -11.84 | 269.63 | 6.25 | 201.35 | 0.2939 | 985.0 | 775.1 | |
| 0 | 6 | 0 | 3 | -11.80 | 269.20 | 5.81 | 200.03 | 0.2907 | 1041.0 | 756.5 | |
| 0 | 10 | 0 | 5 | -13.55 | 267.37 | 3.99 | 192.64 | 0.3103 | 1193.0 | 936.9 | |
| 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. | |