| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 65 | 357 | 41 | 227 | -12.14 | 176.04 | -35.52 | 114.62 | 0.6271 | 408.9 | 290.0 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-07 19:11:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -12.14 | 178.65 | -32.91 | 116.17 | 0.5941 | 658.0 | 511.7 | |
| 8 | 246 | 5 | 154 | -13.58 | 177.67 | -33.89 | 117.70 | 0.6144 | 1107.3 | 607.9 | |
| 8 | -2 | 5 | -2 | -12.45 | 177.65 | -33.90 | 116.01 | 0.6083 | 1571.2 | 999999 | |
| 6 | -2 | 4 | -2 | -12.35 | 177.34 | -34.22 | 115.64 | 0.6117 | 1141.1 | 999999 | |
| 8 | -2 | 5 | -2 | -12.64 | 176.96 | -34.60 | 115.85 | 0.6180 | 963.0 | 999999 | |
| 7 | -2 | 4 | -2 | -12.96 | 176.81 | -34.75 | 116.24 | 0.6216 | 898.4 | 999999 | |
| 4 | -2 | 2 | -2 | -12.33 | 176.72 | -34.84 | 115.23 | 0.6193 | 884.8 | 999999 | |
| 5 | -2 | 3 | -2 | -12.83 | 176.01 | -35.55 | 115.56 | 0.6307 | 591.0 | 999999 | |
| 0 | 7 | 0 | 5 | -12.04 | 175.84 | -35.71 | 114.29 | 0.6287 | 513.0 | 482.5 | |
| 0 | 6 | 0 | 4 | -12.18 | 175.43 | -36.12 | 114.26 | 0.6344 | 486.0 | 387.2 | |
| 0 | 3 | 0 | 2 | -10.15 | 174.56 | -37.00 | 110.78 | 0.6359 | -778.0 | -560.2 | |
| 0 | 15 | 0 | 10 | -10.59 | 174.30 | -37.26 | 111.31 | 0.6411 | -1098.0 | -680.5 | |
| 0 | 3 | 0 | 2 | -9.42 | 173.92 | -37.64 | 109.39 | 0.6410 | -805.0 | -649.1 | |
| 6 | 70 | 4 | 46 | -10.43 | 173.48 | -38.08 | 110.67 | 0.6506 | -1042.5 | -492.4 | |
| 8 | -14 | 5 | -14 | -10.64 | 173.10 | -38.46 | 110.80 | 0.6562 | -1028.7 | 999999 | |
| 5 | -14 | 4 | -14 | -10.78 | 172.63 | -38.93 | 110.78 | 0.6626 | -733.7 | 999999 | |
| 0 | 3 | 0 | 2 | -11.05 | 171.72 | -39.84 | 110.75 | 0.6747 | -596.0 | -443.1 | |
| 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. | |