Esempio n. 1
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def extract_semi_major(en):
    shape = (ens.nbod-1,ens.nsys)
    value = numpy.empty(shape)
    for sysid, sys in enumerate(en):
        star = sys[0]
        center = (star.pos,star.vel,star.mass)

        for bodid in range(1,en.nbod):
            bod = sys[bodid]
            planet = (bod.pos,bod.vel,bod.mass)
            orbital_elements = swarmng.keplerian_for_cartesian(planet,center)
            value[bodid-1,sysid] = orbital_elements.a

    return value    
Esempio n. 2
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# * planet number 0 to nbod-1
# * orbital element number : 0 to 5
# * system id
#
import numpy

shape = (ens.nbod-1, 6, ens.nsys)
value = numpy.empty(shape)
for sysid, sys in enumerate(ens):
    star = sys[0]
    center = (star.pos,star.vel,star.mass)

    for bodid in range(1,ens.nbod):
        bod = sys[bodid]
        planet = (bod.pos,bod.vel,bod.mass)
        orbital_elements = swarmng.keplerian_for_cartesian(planet,center)
        value[bodid-1, :,sysid] = orbital_elements

# @section pr Write the information to standard output
# Now iterate through the 3-dimensional array
# and calculate the average and standard deviation
# of each orbital element value for each body, then
# print it to the output.
#
print("Body number, Semi-major axis, Eccentricity, Inclination, Longtitude of the ascending node, Argument of periapsis, Mean anomaly")
for bodid in range(1,ens.nbod):
    orbital_elements = [0,0,0,0,0]
    o = "{0}".format(bodid)
    for i in range(0,6):
      o += ", {0}±{1}".format(numpy.average(value[bodid-1,i,:]),numpy.std(value[bodid-1,i,:]))
    print(o)