本文整理汇总了Python中galpy.orbit.Orbit.rperi方法的典型用法代码示例。如果您正苦于以下问题:Python Orbit.rperi方法的具体用法?Python Orbit.rperi怎么用?Python Orbit.rperi使用的例子?那么恭喜您, 这里精选的方法代码示例或许可以为您提供帮助。您也可以进一步了解该方法所在类galpy.orbit.Orbit
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在下文中一共展示了Orbit.rperi方法的4个代码示例,这些例子默认根据受欢迎程度排序。您可以为喜欢或者感觉有用的代码点赞,您的评价将有助于系统推荐出更棒的Python代码示例。
示例1: test_adinvariance
# 需要导入模块: from galpy.orbit import Orbit [as 别名]
# 或者: from galpy.orbit.Orbit import rperi [as 别名]
def test_adinvariance():
from galpy.potential import IsochronePotential
from galpy.orbit import Orbit
from galpy.actionAngle import actionAngleIsochrone
# Initialize two different IsochronePotentials
ip1= IsochronePotential(normalize=1.,b=1.)
ip2= IsochronePotential(normalize=0.5,b=1.)
# Use TimeInterpPotential to interpolate smoothly
tip= TimeInterpPotential(ip1,ip2,dt=100.,tform=50.)
# Integrate: 1) Orbit in the first isochrone potential
o1= Orbit([1.,0.1,1.1,0.0,0.1,0.])
ts= numpy.linspace(0.,50.,1001)
o1.integrate(ts,tip)
o1.plot(d1='x',d2='y',xrange=[-1.6,1.6],yrange=[-1.6,1.6],
color='b')
# 2) Orbit in the transition
o2= o1(ts[-1]) # Last time step => initial time step
ts2= numpy.linspace(50.,150.,1001)
o2.integrate(ts2,tip)
o2.plot(d1='x',d2='y',overplot=True,color='g')
# 3) Orbit in the second isochrone potential
o3= o2(ts2[-1])
ts3= numpy.linspace(150.,200.,1001)
o3.integrate(ts3,tip)
o3.plot(d1='x',d2='y',overplot=True,color='r')
# Now we calculate energy, maximum height, and mean radius
print(o1.E(pot=ip1), (o1.rperi()+o1.rap())/2, o1.zmax())
assert numpy.fabs(o1.E(pot=ip1)+2.79921356237) < 10.**-4., 'Energy in the adiabatic invariance test is different'
assert numpy.fabs((o1.rperi()+o1.rap())/2-1.07854158141) < 10.**-4., 'mean radius in the adiabatic invariance test is different'
assert numpy.fabs(o1.zmax()-0.106331362938) < 10.**-4., 'zmax in the adiabatic invariance test is different'
print(o3.E(pot=ip2), (o3.rperi()+o3.rap())/2, o3.zmax())
assert numpy.fabs(o3.E(pot=ip2)+1.19677002624) < 10.**-4., 'Energy in the adiabatic invariance test is different'
assert numpy.fabs((o3.rperi()+o3.rap())/2-1.39962036137) < 10.**-4., 'mean radius in the adiabatic invariance test is different'
assert numpy.fabs(o3.zmax()-0.138364269321) < 10.**-4., 'zmax in the adiabatic invariance test is different'
# The orbit has clearly moved to larger radii,
# the actions are however conserved from beginning to end
aAI1= actionAngleIsochrone(ip=ip1); print(aAI1(o1))
js= aAI1(o1)
assert numpy.fabs(js[0]-numpy.array([ 0.00773779])) < 10.**-4., 'action in the adiabatic invariance test is different'
assert numpy.fabs(js[1]-numpy.array([ 1.1])) < 10.**-4., 'action in the adiabatic invariance test is different'
assert numpy.fabs(js[2]-numpy.array([ 0.0045361])) < 10.**-4., 'action in the adiabatic invariance test is different'
aAI2= actionAngleIsochrone(ip=ip2); print(aAI2(o3))
js= aAI2(o3)
assert numpy.fabs(js[0]-numpy.array([ 0.00773812])) < 10.**-4., 'action in the adiabatic invariance test is different'
assert numpy.fabs(js[1]-numpy.array([ 1.1])) < 10.**-4., 'action in the adiabatic invariance test is different'
assert numpy.fabs(js[2]-numpy.array([ 0.0045361])) < 10.**-4., 'action in the adiabatic invariance test is different'
return None
示例2: test_orbmethods
# 需要导入模块: from galpy.orbit import Orbit [as 别名]
# 或者: from galpy.orbit.Orbit import rperi [as 别名]
def test_orbmethods():
from galpy.orbit import Orbit
from galpy.potential import MWPotential2014
o= Orbit([0.8,0.3,0.75,0.,0.2,0.]) # setup R,vR,vT,z,vz,phi
times= numpy.linspace(0.,10.,1001) # Output times
o.integrate(times,MWPotential2014) # Integrate
o.E() # Energy
assert numpy.fabs(o.E()+1.2547650648697966) < 10.**-5., 'Orbit method does not work as expected'
o.L() # Angular momentum
assert numpy.all(numpy.fabs(o.L()-numpy.array([[ 0. , -0.16, 0.6 ]])) < 10.**-5.), 'Orbit method does not work as expected'
o.Jacobi(OmegaP=0.65) #Jacobi integral E-OmegaP Lz
assert numpy.fabs(o.Jacobi(OmegaP=0.65)-numpy.array([-1.64476506])) < 10.**-5., 'Orbit method does not work as expected'
o.ER(times[-1]), o.Ez(times[-1]) # Rad. and vert. E at end
assert numpy.fabs(o.ER(times[-1])+1.27601734263047) < 10.**-5., 'Orbit method does not work as expected'
assert numpy.fabs(o.Ez(times[-1])-0.021252201847851909) < 10.**-5., 'Orbit method does not work as expected'
o.rperi(), o.rap(), o.zmax() # Peri-/apocenter r, max. |z|
assert numpy.fabs(o.rperi()-0.44231993168097) < 10.**-5., 'Orbit method does not work as expected'
assert numpy.fabs(o.rap()-0.87769030382105) < 10.**-5., 'Orbit method does not work as expected'
assert numpy.fabs(o.zmax()-0.077452357289016) < 10.**-5., 'Orbit method does not work as expected'
o.e() # eccentricity (rap-rperi)/(rap+rperi)
assert numpy.fabs(o.e()-0.32982348199330563) < 10.**-5., 'Orbit method does not work as expected'
o.R(2.,ro=8.) # Cylindrical radius at time 2. in kpc
assert numpy.fabs(o.R(2.,ro=8.)-3.5470772876920007) < 10.**-3., 'Orbit method does not work as expected'
o.vR(5.,vo=220.) # Cyl. rad. velocity at time 5. in km/s
assert numpy.fabs(o.vR(5.,vo=220.)-45.202530965094553) < 10.**-3., 'Orbit method does not work as expected'
o.ra(1.), o.dec(1.) # RA and Dec at t=1. (default settings)
# 5/12/2016: test weakened, because improved galcen<->heliocen
# transformation has changed these, but still close
assert numpy.fabs(o.ra(1.)-numpy.array([ 288.19277])) < 10.**-1., 'Orbit method does not work as expected'
assert numpy.fabs(o.dec(1.)-numpy.array([ 18.98069155])) < 10.**-1., 'Orbit method does not work as expected'
o.jr(type='adiabatic'), o.jz() # R/z actions (ad. approx.)
assert numpy.fabs(o.jr(type='adiabatic')-0.05285302231137586) < 10.**-3., 'Orbit method does not work as expected'
assert numpy.fabs(o.jz()-0.006637988850751242) < 10.**-3., 'Orbit method does not work as expected'
# Rad. period w/ Staeckel approximation w/ focal length 0.5,
o.Tr(type='staeckel',delta=0.5,ro=8.,vo=220.) # in Gyr
assert numpy.fabs(o.Tr(type='staeckel',delta=0.5,ro=8.,vo=220.)-0.1039467864018446) < 10.**-3., 'Orbit method does not work as expected'
o.plot(d1='R',d2='z') # Plot the orbit in (R,z)
o.plot3d() # Plot the orbit in 3D, w/ default [x,y,z]
return None
示例3: illustrate_adiabatic_invariance
# 需要导入模块: from galpy.orbit import Orbit [as 别名]
# 或者: from galpy.orbit.Orbit import rperi [as 别名]
def illustrate_adiabatic_invariance(plotfilename1,plotfilename2):
# Initialize two different IsochronePotentials
ip1= IsochronePotential(normalize=1.,b=1.)
ip2= IsochronePotential(normalize=0.5,b=1.)
# Use TimeInterpPotential to interpolate smoothly between the two
tip= TimeInterpPotential(ip1,ip2,dt=100.,tform=50.)
# Integrate the orbit, in three parts
# 1) Orbit in the first isochrone potential
o1= Orbit([1.,0.1,1.1,0.0,0.1,0.])
ts= numpy.linspace(0.,50.,1001)
o1.integrate(ts,tip)
bovy_plot.bovy_print()
o1.plot(d1='x',d2='y',xrange=[-1.6,1.6],yrange=[-1.6,1.6],color='b',
gcf=True)
# 2) Orbit in the transition
o2= o1(ts[-1]) # Last time step = initial time step of the next integration
ts2= numpy.linspace(50.,150.,1001)
o2.integrate(ts2,tip)
o2.plot(d1='x',d2='y',overplot=True,color='g')
# 3) Orbit in the second isochrone potential
o3= o2(ts2[-1])
ts3= numpy.linspace(150.,200.,1001)
o3.integrate(ts3,ip2)
o3.plot(d1='x',d2='y',overplot=True,color='r')
bovy_plot.bovy_end_print(plotfilename1)
# Also plot the R,z projection
bovy_plot.bovy_print(fig_height=2.3333)
o1.plot(d1='R',d2='z',xrange=[0.9,1.65],yrange=[-.175,.175],color='b',
gcf=True)
o2.plot(d1='R',d2='z',overplot=True,color='g')
o3.plot(d1='R',d2='z',overplot=True,color='r')
bovy_plot.bovy_end_print(plotfilename2)
# Now we calculate the energy, eccentricity, mean radius, and maximum height
print o1.E(pot=ip1), o1.e(), 0.5*(o1.rperi()+o1.rap()), o1.zmax()
print o3.E(pot=ip2), o3.e(), 0.5*(o3.rperi()+o3.rap()), o3.zmax()
# The orbit has clearly moved to larger radii, the actions are however conserved
aAI1= actionAngleIsochrone(ip=ip1)
aAI2= actionAngleIsochrone(ip=ip2)
print aAI1(o1)
print aAI2(o3)
return None
示例4: calcOrbits
# 需要导入模块: from galpy.orbit import Orbit [as 别名]
# 或者: from galpy.orbit.Orbit import rperi [as 别名]
def calcOrbits(parser):
options,args= parser.parse_args()
#Read data
XYZ,vxvyvz,cov_vxvyvz,rawdata= readData(metal='allall',
sample=options.sample,
loggmin=4.2,
snmin=15.,
select=options.select)
#Define potential
if options.logp:
pot= LogarithmicHaloPotential(normalize=1.)
else:
pot= MWPotential
ts= numpy.linspace(0.,_MAXT,10000) #times to integrate
if os.path.exists(args[0]):#Load savefile
savefile= open(args[0],'rb')
orbits= pickle.load(savefile)
_ORBITSLOADED= True
try:
samples= pickle.load(savefile)
except EORError:
_SAMPLESLOADED= False
else:
_SAMPLESLOADED= True
finally:
savefile.close()
else:
_ORBITSLOADED= False
if not _ORBITSLOADED:
#First calculate orbits
es, rmeans, rperis, raps, zmaxs = [], [], [], [], []
densrmeans, vzrmeans= [], []
for ii in range(len(rawdata)):
sys.stdout.write('\r'+"Working on object %i/%i" % (ii,len(rawdata)))
sys.stdout.flush()
#Integrate the orbit
data= rawdata[ii]
o= Orbit([data.ra,data.dec,data.dist,data.pmra,data.pmdec,data.vr],
radec=True,vo=220.,ro=8.,zo=_ZSUN)
o.integrate(ts,pot)
es.append(o.e())
rperis.append(o.rperi())
raps.append(o.rap())
zmaxs.append(o.zmax())
rmeans.append(0.5*(o.rperi()+o.rap()))
Rs= o.R(ts)
vz2= o.vz(ts)**2.
dens= evaluateDensities(Rs,0.*Rs,pot)
densrmeans.append(numpy.sum(dens*Rs)/numpy.sum(dens))
vzrmeans.append(numpy.sum(vz2*Rs)/numpy.sum(vz2))
# print " ", rmeans[-1], densrmeans[-1], vzrmeans[-1]
sys.stdout.write('\r'+_ERASESTR+'\r')
sys.stdout.flush()
es= numpy.array(es)
rmeans= numpy.array(rmeans)
rperis= numpy.array(rperis)
raps= numpy.array(raps)
zmaxs= numpy.array(zmaxs)
orbits= _append_field_recarray(rawdata,'e',es)
orbits= _append_field_recarray(orbits,'rmean',rmeans)
orbits= _append_field_recarray(orbits,'rperi',rperis)
orbits= _append_field_recarray(orbits,'rap',raps)
orbits= _append_field_recarray(orbits,'zmax',zmaxs)
orbits= _append_field_recarray(orbits,'densrmean',densrmeans)
orbits= _append_field_recarray(orbits,'vzrmean',vzrmeans)
#Pickle
savefile= open(args[0],'wb')
pickle.dump(orbits,savefile)
savefile.close()
return None