SOHO MDI 2000-11-05 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 76 | 0 | 43 | 10.64 | 267.23 | 30.20 | 285.52 | 0.5133 | 169.2 | 139.6 | |
|
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 | 5 | 0 | 3 | 6.28 | 275.60 | 38.56 | 275.33 | 0.6247 | 621.0 | 622.9 | |
| 0 | 4 | 0 | 3 | 10.65 | 273.54 | 36.51 | 282.76 | 0.6018 | 506.0 | 520.6 | |
| 0 | 3 | 0 | 2 | 10.43 | 273.27 | 36.23 | 282.45 | 0.5976 | 583.0 | 594.2 | |
| 0 | 4 | 0 | 2 | 9.43 | 272.13 | 35.10 | 281.00 | 0.5800 | 403.0 | 451.5 | |
| 0 | 6 | 0 | 3 | 9.99 | 271.48 | 34.45 | 282.12 | 0.5720 | 777.0 | 606.5 | |
| 0 | 7 | 0 | 4 | 9.79 | 269.58 | 32.55 | 282.23 | 0.5447 | 653.0 | 662.1 | |
| 0 | 3 | 0 | 2 | 8.90 | 269.49 | 32.46 | 280.62 | 0.5416 | -346.0 | -191.6 | |
| 0 | 2 | 0 | 1 | 10.37 | 269.55 | 32.52 | 283.30 | 0.5456 | 598.0 | 518.5 | |
| 0 | 10 | 0 | 6 | 9.64 | 269.42 | 32.39 | 281.99 | 0.5421 | 1012.0 | 842.5 | |
| 0 | 4 | 0 | 2 | 11.63 | 266.95 | 29.92 | 286.54 | 0.5117 | 503.0 | 415.9 | |
| 0 | 6 | 0 | 3 | 11.89 | 261.92 | 24.89 | 289.65 | 0.4392 | -695.0 | -643.8 | |
| 0 | 9 | 0 | 5 | 12.26 | 261.44 | 24.41 | 290.77 | 0.4337 | -751.0 | -727.9 | |
| 0 | 5 | 0 | 3 | 12.24 | 260.71 | 23.67 | 291.23 | 0.4228 | -858.0 | -807.1 | |
| 0 | 8 | 0 | 4 | 13.78 | 256.47 | 19.44 | 298.74 | 0.3703 | -637.0 | -504.2 | |
| 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. | |