Table 5:
Summary of the parameters used to compute the spectrum in 2D geometry
using the Busche & Hillier (2005) code. Note that the density contrast between equator and pole is given by 1+a for oblate models, and 1/(1+a) for prolate models.
| Model |
Density |
a |
b |
Velocity |
VB1 |
VB2 |
VB3 |
| |
profile |
|
|
changes? |
|
|
|
|
1 |
oblate |
1 |
2 |
no |
... |
... |
... |
|
2 |
prolate |
1 |
2 |
no |
... |
... |
... |
|
3 |
oblate |
3 |
2 |
no |
... |
... |
... |
|
4 |
oblate |
3 |
5 |
no |
... |
... |
... |
|
5 |
oblate |
7 |
2 |
no |
... |
... |
... |
|
6 |
oblate |
7 |
5 |
no |
... |
... |
... |
|
7 |
oblate |
15 |
2 |
no |
... |
... |
... |
|
8 |
none |
... |
... |
yes |
0.2 |
0.8 |
4 |
|
9 |
oblate |
3 |
2 |
yes |
0.8 |
2.2 |
4 |
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