| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28 | 190 | 44 | 294 | -23.19 | 304.70 | 67.67 | 243.91 | 0.9472 | -171.9 | -82.9 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-05 20:47:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 5 | -19.90 | 305.18 | 68.15 | 247.43 | 0.9466 | -217.0 | -260.4 | |
| 0 | 12 | 0 | 22 | -22.71 | 307.92 | 70.89 | 245.07 | 0.9624 | -37.0 | -125.5 | |
| 3 | 10 | 4 | 15 | -20.50 | 304.85 | 67.82 | 246.74 | 0.9455 | -268.2 | -151.7 | |
| 0 | 4 | 0 | 6 | -20.60 | 303.75 | 66.72 | 246.41 | 0.9398 | -291.0 | -304.5 | |
| 0 | 3 | 0 | 4 | -20.10 | 303.12 | 66.09 | 246.79 | 0.9356 | -321.0 | -296.0 | |
| 5 | 106 | 9 | 175 | -24.17 | 306.67 | 69.64 | 243.34 | 0.9584 | 95.2 | -86.3 | |
| 0 | 15 | 0 | 21 | -21.44 | 303.15 | 66.12 | 245.40 | 0.9376 | -473.0 | -420.7 | |
| 13 | -6 | 22 | -6 | -24.10 | 305.64 | 68.60 | 243.20 | 0.9536 | -467.9 | 999999 | |
| 0 | 4 | 0 | 5 | -20.32 | 299.92 | 62.89 | 245.83 | 0.9167 | 235.0 | 154.7 | |
| 4 | 12 | 5 | 15 | -21.79 | 300.04 | 63.01 | 244.30 | 0.9199 | 244.6 | 117.3 | |
| 0 | 3 | 0 | 4 | -22.81 | 299.29 | 62.26 | 243.04 | 0.9171 | 358.0 | 238.6 | |
| 3 | 10 | 4 | 13 | -23.45 | 299.46 | 62.43 | 242.40 | 0.9194 | 365.5 | 265.2 | |
| 0 | 6 | 0 | 7 | -23.43 | 297.67 | 60.64 | 241.93 | 0.9081 | 142.0 | 194.0 | |
| 0 | 2 | 0 | 2 | -23.83 | 297.90 | 60.87 | 241.57 | 0.9104 | 358.0 | 312.8 | |
| 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. | |