SOHO MDI 2000-11-01 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67 | 476 | 39 | 276 | -23.20 | 305.75 | 16.01 | 208.97 | 0.5256 | -1222.4 | -627.6 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-01 20:47:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -20.95 | 310.46 | 20.72 | 218.15 | 0.5371 | -595.0 | -535.5 | |
| 5 | 13 | 3 | 7 | -23.34 | 308.20 | 18.47 | 212.36 | 0.5456 | -601.1 | -406.9 | |
| 18 | 117 | 10 | 68 | -22.41 | 307.37 | 17.64 | 212.19 | 0.5278 | -1639.0 | -760.7 | |
| 0 | 5 | 0 | 3 | -24.01 | 306.88 | 17.15 | 209.83 | 0.5437 | -440.0 | -328.2 | |
| 0 | 6 | 0 | 4 | -24.97 | 306.58 | 16.84 | 208.45 | 0.5534 | -488.0 | -416.8 | |
| 3 | 10 | 2 | 6 | -22.60 | 305.96 | 16.22 | 209.91 | 0.5192 | -1210.6 | -903.0 | |
| 0 | 7 | 0 | 4 | -25.13 | 306.16 | 16.42 | 207.71 | 0.5526 | -661.0 | -507.6 | |
| 22 | 170 | 13 | 99 | -23.89 | 305.59 | 15.86 | 208.07 | 0.5330 | -1401.9 | -602.0 | |
| 0 | 2 | 0 | 1 | -25.21 | 305.55 | 15.81 | 206.77 | 0.5494 | 186.0 | 224.5 | |
| 0 | 6 | 0 | 3 | -22.93 | 305.17 | 15.43 | 208.38 | 0.5177 | -1045.0 | -815.2 | |
| 14 | -8 | 8 | -8 | -23.57 | 304.99 | 15.25 | 207.47 | 0.5248 | -1451.8 | 999999 | |
| 0 | 8 | 0 | 5 | -22.49 | 304.82 | 15.08 | 208.28 | 0.5095 | -1042.0 | -909.5 | |
| 5 | 37 | 3 | 22 | -25.55 | 304.97 | 15.23 | 205.64 | 0.5501 | 461.2 | -27.9 | |
| 0 | 78 | 0 | 44 | -22.09 | 304.30 | 14.56 | 207.86 | 0.5007 | -1300.0 | -867.1 | |
| 0 | 5 | 0 | 3 | -21.21 | 303.19 | 13.45 | 206.90 | 0.4812 | -624.0 | -469.8 | |
| 0 | 5 | 0 | 3 | -22.11 | 303.15 | 13.41 | 205.95 | 0.4930 | 317.0 | 123.1 | |
| 0 | 3 | 0 | 2 | -20.91 | 302.78 | 13.04 | 206.51 | 0.4743 | -776.0 | -651.7 | |
| 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. | |