Tidal & Coriolis Test

Physical Parameters

1.32443x10-16 g/cc
0.263435 MJ
1.350 Msun
(0.04747, 0, 0) AU
1.95 rad/day
2.65 RP
lRotateT
lStellarGravityT

Simulation Parameters

BaseRes(32, 32, 32)
MaxLevel3

Fixed boundary (old code)

1x10-19 g/cc
102 K
104 K
2.6369
lPlanetTempProfileT

set such that RP is equal for both runs.

Zones/RP~27
Extent(.9, -.1, -.1, 1.1, .1, .1)
Physical Extent(6.381x1011, -7.09x1010, -7.09x1010, 7.799x1011, 7.09x1010, 7.09x1010) cm


TimeScale3.52 days
lScale7.09x1011 cm

TimeScale = Porb
lScale = a

http://www.pas.rochester.edu/~adebrech/PlanetIonization/rot_test/fixed_boundary_side0010.png

http://www.pas.rochester.edu/~adebrech/PlanetIonization/rot_test/fixed_boundary_top0010.png

Contour key:

PurpleMach 1 surface
LilacMach 10 surface
BlackExtent of box below
RedRP
WhiteRHill
Brownish-red

Not enough frames to capture evolution (where I suspect the tidal forces may be apparent). Requeued with 1/10th time. However, top view shows clear Coriolis effect. Looks perhaps a bit stronger but otherwise consistent with and given Fig. 6.

Line Transfer

3x103 K
2.14559 RJ
lRampFluxT
HalfTime4
RampSpeed2.65
Fluxmax2x1013 phot/cm2/s


Zones/RP32
Extent(43, -4, -4, 51, 4, 4)
Physical Extent(6.45x1011, -6x1010, -6x1010, 7.65x1011, 6x1010, 6x1010) cm
frames/CT100


TimeScale8.3825 hours
lScale1.5x1010 cm

lScale = RP

http://www.pas.rochester.edu/~adebrech/PlanetIonization/rot_test/rot_test_side0820.png

http://www.pas.rochester.edu/~adebrech/PlanetIonization/rot_test/rot_test_top0820.png

Contour key:

PurpleMach 1 surface
Black
GreenRib
RedRP
YellowRob
Brownish-red

Unable to start from steady-state run, planet in incorrect position. At frame 760, there still appears to be some subsonic material at the edges, but this may just be because it hasn't yet blown out the entire ambient. The flow profile seems to be more strongly entrained up- and downwind than the above run.

Next?

May be best to run a (slightly larger?) box to steady state with the planet located correctly (using HD209458b orbital parameters - appropriate?), then add stellar gravity and rotation.

Comments

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