M-9
![http://www.pas.rochester.edu/~bliu/pnStudy/M2-9/M2-9.1952-2015.jpg http://www.pas.rochester.edu/~bliu/pnStudy/M2-9/M2-9.1952-2015.jpg](http://www.pas.rochester.edu/~bliu/pnStudy/M2-9/M2-9.1952-2015.jpg)
Test 1 9.30.2015
The shape depends on the resolution. See the non-pulsed result with different resolution:
*3D
Test 2
if(lPulsed) then
qjet(1)=qjet(1)*(abs(cos(Omega_Pulsed*time))**PulseModule)
end if
&ProblemData
! MODEL: jet 0deg (n=4e4, r=1000AU, T=100K) @ 200 km/s into 4e4 torus + AGB wind
! folder taper15n4e2v200namb4e4
!
! BACKGROUND or “AMBIENT” SECTION. Values apply to origin
tamb = 1d3 ! ambient temp, 1cu = 0.1K (100K=1000cu)
namb = 4e4 ! ambient central density cm^-3. Usually 400 for 1/r^2 or torus.
stratified = t ! true = add a 1/r^2 background 'AGB stellar wind'
torus = f ! true - add torus to the background
torusalpha = 0.7 ! alpha and beta specify the geometry
torusbeta = 10d0 ! see Frank & Mellema, 1994ApJ...430..800F
rings = f ! true - add radial density modulations to AGB wind
!
! FLOW DESCRIPTION SECTION, values apply at origin at t=0
outflowType = 2 ! TYPE OF FLOW 1 cyl jet, 2 conical wind, 3 is clump
njet = 4d4 ! flow density at launch zone, 1cu = 1cm^-3
Rjet = 2d0 ! flow radius at launch zone, 1cu = 500AU (outflowType=1 only)
vjet = 2e7 ! flow velocity , 1cu = cm/s (100km/s=1e7cu)
tjet = 1d3 ! flow temp, 1cu = 0.1K (100K=1000cu)
tt = 0.0d0 ! flow accel time, 1cu = 8250y (0.02 = 165y)
open_angle = 15d0 ! conical flow open angle (deg)
tf = 15d0 ! conical flow Gaussian taper (deg) for njet and vjet; 0= disable
sigma = 0d0 ! !toroidal.magnetic.energy / kinetic.energy, example 0.6
!
! OTHER PARAMETERS
lcooling = t ! radiative cooling?
buff = 8 ! central refinement of a grid with a resolution 1/2
! for Taper
lObliqueCone = F !T, 45 deg tamper
!F, non 45 deg tamper
! for M2-9 Pulsed jet (density)
lPulsed = T !T, turn on pulsed jet
!F, turn off
PulsedPeriod = 150 ! year
PulseModule = 4 ! 1 abs(cos)
! 2 abs(cos)^2
! 4 abs(cos)^4
/