| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 106 | 784 | 56 | 409 | 2.53 | 271.70 | -18.04 | 94.79 | 0.3117 | 1747.5 | 667.4 | |
|
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 |
| 32 | 708 | 17 | 368 | 2.26 | 272.96 | -16.77 | 96.11 | 0.2913 | 2197.3 | 696.8 | |
| 0 | 5 | 0 | 3 | 4.21 | 272.61 | -17.13 | 89.34 | 0.2951 | 116.0 | 209.6 | |
| 22 | -1 | 12 | -1 | 2.17 | 272.44 | -17.30 | 96.19 | 0.3002 | 1580.6 | 999999 | |
| 0 | 9 | 0 | 5 | 0.85 | 272.09 | -17.65 | 100.29 | 0.3095 | 817.0 | 607.1 | |
| 11 | -1 | 6 | -1 | 3.39 | 272.02 | -17.72 | 92.02 | 0.3054 | 1647.4 | 999999 | |
| 7 | -1 | 3 | -1 | 2.38 | 271.63 | -18.11 | 95.19 | 0.3132 | 1228.5 | 999999 | |
| 30 | -1 | 16 | -1 | 2.92 | 271.58 | -18.16 | 93.45 | 0.3132 | 1736.2 | 999999 | |
| 0 | 6 | 0 | 3 | 0.53 | 271.56 | -18.17 | 100.97 | 0.3191 | 682.0 | 524.2 | |
| 4 | -1 | 2 | -1 | 2.83 | 271.22 | -18.52 | 93.63 | 0.3193 | 1320.3 | 999999 | |
| 0 | 4 | 0 | 2 | 4.38 | 268.35 | -21.39 | 88.73 | 0.3653 | -530.0 | -417.7 | |
| 0 | 9 | 0 | 5 | 3.11 | 266.92 | -22.81 | 91.98 | 0.3891 | 809.0 | 661.0 | |
| 0 | 10 | 0 | 5 | 0.71 | 266.62 | -23.12 | 97.99 | 0.3981 | 859.0 | 696.8 | |
| 0 | 19 | 0 | 10 | 2.25 | 266.44 | -23.30 | 94.08 | 0.3980 | 767.0 | 668.3 | |
| 0 | 5 | 0 | 3 | 1.43 | 263.56 | -26.17 | 95.31 | 0.4448 | 694.0 | 537.8 | |
| 0 | 9 | 0 | 5 | 2.70 | 259.06 | -30.67 | 91.81 | 0.5119 | -738.0 | -592.3 | |
| 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. | |