def testProperMotion(self):
"""Convert.proper_motion: multiple V6C values."""
ra = tpm.d2r(269.45402305)
de = tpm.d2r(4.66828815)
px = 549.01 / 1000.0 # To Arc seconds
rv = 0.0
# pmra * cos(de) into pmra
pmra = (-797.84 / 1000.0) / math.cos(de)
pmra *= 100.0 # To Arcseconds per century.
pmde = (10326.93 / 1000.0)
pmde *= 100.0 # To Arcseconds per century.
C = tpm.CJ
v6 = tpm.cat2v6(ra, de, pmra, pmde, px, rv, C)
v6_out = convert.proper_motion([v6, v6], tpm.J2000,
tpm.jyear2jd(1991.25))
for i in v6_out:
v6 = i.c2s()
hms = tpm.HMS(r=v6.alpha)
dms = tpm.DMS(r=v6.delta)
hms.normalize()
dms.normalize()
self.assertAlmostEqual(hms.hh, -7.0)
self.assertAlmostEqual(hms.mm, 57.0)
self.assertAlmostEqual(hms.ss, 48.4986, 3)
self.assertAlmostEqual(dms.dd, 4.0)
self.assertAlmostEqual(dms.mm, 41.0)
self.assertAlmostEqual(dms.ss, 36.1980, 3)
def testProperMotion(self):
"""Convert.proper_motion: multiple V6C values."""
ra = tpm.d2r(269.45402305)
de = tpm.d2r(4.66828815)
px = 549.01 / 1000.0 # To Arc seconds
rv = 0.0
# pmra * cos(de) into pmra
pmra = (-797.84 / 1000.0) / math.cos(de)
pmra *= 100.0 # To Arcseconds per century.
pmde = 10326.93 / 1000.0
pmde *= 100.0 # To Arcseconds per century.
C = tpm.CJ
v6 = tpm.cat2v6(ra, de, pmra, pmde, px, rv, C)
v6_out = convert.proper_motion([v6, v6], tpm.J2000, tpm.jyear2jd(1991.25))
for i in v6_out:
v6 = i.c2s()
hms = tpm.HMS(r=v6.alpha)
dms = tpm.DMS(r=v6.delta)
hms.normalize()
dms.normalize()
self.assertAlmostEqual(hms.hh, -7.0)
self.assertAlmostEqual(hms.mm, 57.0)
self.assertAlmostEqual(hms.ss, 48.4986, 3)
self.assertAlmostEqual(dms.dd, 4.0)
self.assertAlmostEqual(dms.mm, 41.0)
self.assertAlmostEqual(dms.ss, 36.1980, 3)
def testpm(self):
"""Proper motion => apply PM to position."""
import math
ra = tpm.d2r(269.45402305)
de = tpm.d2r(4.66828815)
px = 549.01 / 1000.0 # To Arc seconds
rv = 0.0
# pmra * cos(de) into pmra
pmra = (-797.84 / 1000.0) / math.cos(de)
pmra *= 100.0 # To Arcseconds per century.
pmde = 10326.93 / 1000.0
pmde *= 100.0 # To Arcseconds per century.
C = tpm.CJ
v6 = tpm.cat2v6(ra, de, pmra, pmde, px, rv, C)
v6 = tpm.proper_motion(v6, tpm.J2000, tpm.jyear2jd(1991.25))
v6 = v6.c2s()
hms = tpm.HMS(r=v6.alpha)
dms = tpm.DMS(r=v6.delta)
hms.normalize()
dms.normalize()
self.assertAlmostEqual(hms.hh, -7.0)
self.assertAlmostEqual(hms.mm, 57.0)
self.assertAlmostEqual(hms.ss, 48.4986, 3)
self.assertAlmostEqual(dms.dd, 4.0)
self.assertAlmostEqual(dms.mm, 41.0)
self.assertAlmostEqual(dms.ss, 36.1980, 3)
def testpm(self):
"""Proper motion => apply PM to position."""
import math
ra = tpm.d2r(269.45402305)
de = tpm.d2r(4.66828815)
px = 549.01 / 1000.0 # To Arc seconds
rv = 0.0
# pmra * cos(de) into pmra
pmra = (-797.84 / 1000.0 ) / math.cos(de)
pmra *= 100.0 # To Arcseconds per century.
pmde = (10326.93 / 1000.0)
pmde *= 100.0 # To Arcseconds per century.
C = tpm.CJ
v6 = tpm.cat2v6(ra, de, pmra, pmde, px, rv, C)
v6 = tpm.proper_motion(v6, tpm.J2000, tpm.jyear2jd(1991.25))
v6 = v6.c2s()
hms = tpm.HMS(r=v6.alpha)
dms = tpm.DMS(r=v6.delta)
hms.normalize()
dms.normalize()
self.assertAlmostEqual(hms.hh, -7.0)
self.assertAlmostEqual(hms.mm, 57.0)
self.assertAlmostEqual(hms.ss, 48.4986, 3)
self.assertAlmostEqual(dms.dd, 4.0)
self.assertAlmostEqual(dms.mm, 41.0)
self.assertAlmostEqual(dms.ss, 36.1980, 3)
def get_state(system):
# The table of TPM states is here
# http://phn.github.com/pytpm/conversions.html#function-convert-convertv6
# We set the epoch and equinox to get consistent results with
# astrolib.coords.Position, see Position._set_tpmstate there.
d = dict()
d['fk5'] = dict(state=tpm.TPM_S06, epoch=tpm.J2000, equinox=tpm.J2000)
d['fk4'] = dict(state=tpm.TPM_S05, epoch=tpm.B1950, equinox=tpm.B1950)
d['galactic'] = dict(state=tpm.TPM_S04, epoch=tpm.J2000, equinox=tpm.byear2jd(1958))
d['ecliptic'] = dict(state=tpm.TPM_S03, epoch=tpm.J2000, equinox=tpm.jyear2jd(1984))
# d['icrs'] = TPM_S06
return d[system]
def get_state(system):
# The table of TPM states is here
# http://phn.github.com/pytpm/conversions.html#function-convert-convertv6
# We set the epoch and equinox to get consistent results with
# astrolib.coords.Position, see Position._set_tpmstate there.
d = dict()
d['fk5'] = dict(state=tpm.TPM_S06, epoch=tpm.J2000, equinox=tpm.J2000)
d['fk4'] = dict(state=tpm.TPM_S05, epoch=tpm.B1950, equinox=tpm.B1950)
d['galactic'] = dict(state=tpm.TPM_S04,
epoch=tpm.J2000,
equinox=tpm.byear2jd(1958))
d['ecliptic'] = dict(state=tpm.TPM_S03,
epoch=tpm.J2000,
equinox=tpm.jyear2jd(1984))
# d['icrs'] = TPM_S06
return d[system]
def testJyear2Jd(self):
"""tpm.jyear2jd() => convert Julian year into Julian date."""
self.assertAlmostEqual(tpm.jyear2jd(2000.0), tpm.J2000)
def testJyear2Jd(self):
"""tpm.jyear2jd() => convert Julian year into Julian date."""
self.assertAlmostEqual(tpm.jyear2jd(2000.0), tpm.J2000)