| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 169 | 987 | 112 | 663 | -11.98 | 350.96 | 38.05 | 243.60 | 0.6722 | 140.8 | 100.8 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-10-03 19:11:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19 | 294 | 14 | 220 | -11.14 | 358.84 | 45.93 | 249.06 | 0.7572 | -786.0 | -418.1 | |
| 26 | -1 | 20 | -1 | -11.41 | 358.22 | 45.31 | 248.45 | 0.7515 | -1337.8 | 999999 | |
| -2 | -1 | -2 | -1 | -11.03 | 358.03 | 45.12 | 248.85 | 0.7480 | 999999 | 999999 | |
| 0 | 5 | 0 | 4 | -12.21 | 352.33 | 39.42 | 244.49 | 0.6900 | 618.0 | 596.9 | |
| 0 | 6 | 0 | 4 | -12.68 | 350.98 | 38.07 | 243.07 | 0.6771 | 163.0 | 155.0 | |
| 0 | 5 | 0 | 3 | -12.13 | 350.68 | 37.77 | 243.64 | 0.6707 | -769.0 | -664.0 | |
| 13 | 115 | 9 | 77 | -12.93 | 350.42 | 37.51 | 242.39 | 0.6720 | -914.2 | -522.8 | |
| 6 | -7 | 4 | -7 | -12.49 | 350.09 | 37.18 | 242.77 | 0.6658 | -1241.6 | 999999 | |
| 8 | 35 | 5 | 22 | -10.76 | 349.13 | 36.22 | 244.59 | 0.6449 | -1159.1 | -832.7 | |
| 0 | 22 | 0 | 14 | -11.57 | 348.51 | 35.60 | 243.05 | 0.6421 | -453.0 | -431.4 | |
| 0 | 5 | 0 | 3 | -10.50 | 348.36 | 35.45 | 244.47 | 0.6342 | -740.0 | -556.7 | |
| 0 | 3 | 0 | 2 | -14.21 | 348.70 | 35.79 | 239.54 | 0.6600 | 378.0 | 295.2 | |
| 0 | 19 | 0 | 12 | -11.98 | 348.03 | 35.12 | 242.14 | 0.6389 | -54.0 | 24.1 | |
| 4 | 45 | 2 | 29 | -13.49 | 347.93 | 35.02 | 239.97 | 0.6469 | 712.5 | 559.5 | |
| 0 | 6 | 0 | 4 | -11.69 | 347.31 | 34.40 | 242.07 | 0.6285 | 206.0 | 210.1 | |
| 0 | 3 | 0 | 2 | -13.17 | 347.49 | 34.58 | 240.10 | 0.6398 | 768.0 | 712.9 | |
| 6 | 17 | 4 | 11 | -12.13 | 347.13 | 34.22 | 241.32 | 0.6291 | 791.1 | 607.4 | |
| 8 | -14 | 5 | -14 | -13.79 | 347.40 | 34.49 | 239.19 | 0.6426 | 895.7 | 999999 | |
| 4 | 389 | 3 | 244 | -11.46 | 346.89 | 33.98 | 242.11 | 0.6221 | 790.0 | 781.8 | |
| 0 | 7 | 0 | 5 | -13.19 | 347.06 | 34.15 | 239.77 | 0.6348 | 730.0 | 625.3 | |
| 6 | -19 | 4 | -19 | -11.30 | 346.30 | 33.39 | 241.92 | 0.6139 | 1013.8 | 999999 | |
| 0 | 11 | 0 | 7 | -10.38 | 345.95 | 33.04 | 243.02 | 0.6040 | 685.0 | 592.9 | |
| 4 | -19 | 3 | -19 | -12.10 | 346.08 | 33.17 | 240.60 | 0.6163 | 1097.8 | 999999 | |
| 14 | -19 | 8 | -19 | -11.83 | 345.80 | 32.89 | 240.77 | 0.6113 | 1531.7 | 999999 | |
| 4 | -19 | 2 | -19 | -12.99 | 345.87 | 32.96 | 239.17 | 0.6197 | 1046.0 | 999999 | |
| 12 | -19 | 7 | -19 | -12.28 | 345.72 | 32.81 | 240.07 | 0.6133 | 1615.0 | 999999 | |
| 6 | -19 | 4 | -19 | -12.73 | 345.69 | 32.78 | 239.40 | 0.6159 | 1222.0 | 999999 | |
| 9 | -19 | 5 | -19 | -11.53 | 345.43 | 32.52 | 240.95 | 0.6049 | 1701.2 | 999999 | |
| 20 | -19 | 13 | -19 | -13.46 | 345.61 | 32.70 | 238.30 | 0.6199 | 1130.4 | 999999 | |
| 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. | |