| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 119 | 1159 | 199 | 2258 | 10.17 | 78.14 | -76.21 | 81.30 | 0.9655 | 454.4 | 24.9 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-09-18 12:47:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 7 | 0 | 12 | 12.95 | 80.33 | -74.02 | 78.59 | 0.9571 | 63.0 | 71.8 | |
| 27 | 943 | 43 | 1566 | 9.58 | 82.28 | -72.07 | 82.26 | 0.9482 | 740.1 | 44.6 | |
| 27 | -2 | 42 | -2 | 10.15 | 81.70 | -72.65 | 81.62 | 0.9511 | 601.3 | 999999 | |
| 20 | -2 | 31 | -2 | 8.98 | 82.20 | -72.15 | 82.89 | 0.9489 | 650.0 | 999999 | |
| -2 | -2 | -2 | -2 | 9.33 | 81.48 | -72.87 | 82.46 | 0.9526 | 999999 | 999999 | |
| 12 | -2 | 20 | -2 | 10.09 | 80.48 | -73.88 | 81.59 | 0.9574 | 126.8 | 999999 | |
| 0 | 12 | 0 | 24 | 14.02 | 77.17 | -77.18 | 77.27 | 0.9710 | 123.0 | 150.9 | |
| 9 | -2 | 16 | -2 | 10.34 | 79.25 | -75.10 | 81.23 | 0.9632 | 305.4 | 999999 | |
| 22 | -2 | 42 | -2 | 10.73 | 78.48 | -75.87 | 80.77 | 0.9665 | 214.1 | 999999 | |
| 0 | 10 | 0 | 23 | 13.94 | 74.82 | -79.54 | 77.18 | 0.9797 | -97.0 | -58.5 | |
| 0 | 28 | 0 | 100 | 14.94 | 70.74 | -83.61 | 75.82 | 0.9910 | -296.0 | -310.9 | |
| 0 | 18 | 0 | 71 | 13.71 | 70.25 | -84.10 | 77.02 | 0.9923 | -200.0 | 112.1 | |
| 0 | 4 | 0 | 11 | 12.57 | 72.49 | -81.86 | 78.38 | 0.9872 | -113.0 | -138.6 | |
| 2 | 33 | 5 | 85 | 8.27 | 74.67 | -79.69 | 82.93 | 0.9819 | -427.5 | -427.3 | |
| 0 | 14 | 0 | 56 | 10.89 | 70.32 | -84.03 | 79.85 | 0.9927 | 152.0 | 294.9 | |
| 0 | 2 | 0 | 8 | 11.18 | 69.73 | -84.62 | 79.50 | 0.9939 | 197.0 | 206.9 | |
| 0 | 9 | 0 | 26 | 7.23 | 73.60 | -80.75 | 83.88 | 0.9856 | -206.0 | -262.8 | |
| 0 | 60 | 0 | 198 | 8.27 | 72.06 | -82.29 | 82.66 | 0.9894 | -202.0 | 44.2 | |
| 0 | 19 | 0 | 78 | 9.50 | 70.41 | -83.94 | 81.25 | 0.9929 | 190.0 | 308.6 | |
| 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. | |