def test_magnetic_correction(self):
"""
Test magentic_correction function.
Input values based on those defined in DPS; output values calculated to
more significant figures using matlab code specified in the DPS.
OOI (2012). Data Product Specification for Velocity Profile and Echo
Intensity. Document Control Number 1341-00750.
https://alfresco.oceanobservatories.org/ (See: Company Home >> OOI
>> Controlled >> 1000 System Level >>
1341-00750_Data_Product_SPEC_VELPROF_OOI.pdf)
Implemented by Christopher Wingard, April 2013
Modified by Russell Desiderio, April 07, 2014. Changed the rtol values
from 1e4 to 1e-4 to get a fair test. Changed the output values by
adding more significant figures.
"""
# apply the magnetic declination correction.
uu_cor, vv_cor = gfunc.magnetic_correction(16.9604, np.array([0.4413]),
np.array([0.1719]))
# test the transform
self.assertTrue(np.allclose(uu_cor, 0.472251, rtol=1e-4, atol=0))
self.assertTrue(np.allclose(vv_cor, 0.035692, rtol=1e-4, atol=0))
def adcp_earth_northward(u, v, z, lat, lon, dt):
"""
Wrapper function to compute the Northward Velocity Profile (VELPROF-VLN)
from the Earth coordinate transformed data.
"""
# force shapes of inputs to arrays of the correct dimensions
u = np.atleast_2d(u)
v = np.atleast_2d(v)
z = np.atleast_1d(z) / 10. # scale decimeter depth input to meters
lat = np.atleast_1d(lat)
lon = np.atleast_1d(lon)
dt = np.atleast_1d(dt)
# calculate the magnetic declination using the WWM2010 model
theta = magnetic_declination(lat, lon, dt, z)
# iterate through arrays for processing multiple records
vv_cor = np.empty(u.shape)
for indx in range(u.shape[0]):
# apply the magnetic variation correction
ucor, vv_cor[indx, :] = magnetic_correction(theta[indx], u[indx, :], v[indx, :])
# scale northward velocity to m/s
vv_cor = vv_cor / 1000. # mm/s -> m/s
# return the Northward Velocity Profile
return vv_cor
def test_magnetic_correction(self):
"""
Test magentic_correction function.
Input values based on those defined in DPS; output values calculated to
more significant figures using matlab code specified in the DPS.
OOI (2012). Data Product Specification for Velocity Profile and Echo
Intensity. Document Control Number 1341-00750.
https://alfresco.oceanobservatories.org/ (See: Company Home >> OOI
>> Controlled >> 1000 System Level >>
1341-00750_Data_Product_SPEC_VELPROF_OOI.pdf)
Implemented by Christopher Wingard, April 2013
Modified by Russell Desiderio, April 07, 2014. Changed the rtol values
from 1e4 to 1e-4 to get a fair test. Changed the output values by
adding more significant figures.
"""
# apply the magnetic declination correction.
uu_cor, vv_cor = gfunc.magnetic_correction(16.9604, np.array([0.4413]),
np.array([0.1719]))
# test the transform
self.assertTrue(np.allclose(uu_cor, 0.472251, rtol=1e-4, atol=0))
self.assertTrue(np.allclose(vv_cor, 0.035692, rtol=1e-4, atol=0))
def test_magnetic_correction(self):
"""
Test magentic_correction function.
Values based on those defined in DPS:
OOI (2012). Data Product Specification for Velocity Profile and Echo
Intensity. Document Control Number 1341-00750.
https://alfresco.oceanobservatories.org/ (See: Company Home >> OOI
>> Controlled >> 1000 System Level >>
1341-00750_Data_Product_SPEC_VELPROF_OOI.pdf)
Implemented by Christopher Wingard, April 2013
"""
# apply the magnetic declination correction.
uu_cor, vv_cor = gfunc.magnetic_correction(16.9604, np.array([0.4413]),
np.array([0.1719]))
# test the transform
self.assertTrue(np.allclose(uu_cor, 0.4722, rtol=1e4, atol=0))
self.assertTrue(np.allclose(vv_cor, 0.0357, rtol=1e4, atol=0))
def adcp_beam_northward(b1, b2, b3, b4, h, p, r, vf, lat, lon, z, dt):
"""
Description:
Wrapper function to compute the Eastward Velocity Profile (VELPROF-VLN)
from beam coordinate transformed velocity profiles as defined in the
Data Product Specification for Velocity Profile and Echo Intensity -
DCN 1341-00750.
Implemented by:
2013-04-10: Christopher Wingard. Initial code.
2014-02-03: Christopher Wingard. Formatting and adjusting to use
magnetic declination values calulated use the WMM 2010.
Usage:
uu_cor = adcp_beam_eastward(b1, b2, b3, b4, h, p, r, vf, lat, lon, z, dt)
where
uu_corr = east velocity profiles in Earth coordinates corrected for the
magnetic declination (VELPROF-VLE_L1) [mm s-1]
b1 = "beam 1" velocity profiles in beam coordinates (VELPROF-B1_L0) [mm s-1]
b2 = "beam 2" velocity profiles in beam coordinates (VELPROF-B2_L0) [mm s-1]
b3 = "beam 3" velocity profiles in beam coordinates (VELPROF-B3_L0) [mm s-1]
b4 = "beam 4" velocity profiles in beam coordinates (VELPROF-B4_L0) [mm s-1]
h = instrument's uncorrected magnetic heading [degrees]
p = instrument pitch [degrees]
r = instrument roll [degrees]
vf = instrument's vertical orientation (0 = downward looking and
1 = upward looking)
lat = instrument's deployment latitude [decimal degrees]
lon = instrument's deployment longitude [decimal degrees]
z = instrument's pressure sensor reading (depth) [dm]
dt = sample date and time value [seconds since 1900-01-01]
"""
# force shapes of inputs to arrays of the correct dimensions
b1 = np.atleast_2d(b1)
b2 = np.atleast_2d(b2)
b3 = np.atleast_2d(b3)
b4 = np.atleast_2d(b4)
h = np.atleast_1d(h)
p = np.atleast_1d(p)
r = np.atleast_1d(r)
vf = np.atleast_1d(vf)
z = np.atleast_1d(z) / 10. # scale decimeter depth input to meters
lat = np.atleast_1d(lat)
lon = np.atleast_1d(lon)
dt = np.atleast_1d(dt)
# compute the beam to instrument transform
u, v, w, e = adcp_beam2ins(b1, b2, b3, b4)
# calculate the magnetic declination using the WWM2010 model
theta = magnetic_declination(lat, lon, dt, z)
# iterate through arrays for processing multiple records
vv_cor = np.empty((b1.shape))
for indx in range(b1.shape[0]):
# compute the instrument to earth beam transform
uu, vv, ww = adcp_ins2earth(u[indx, :], v[indx, :], w[indx, :],
h[indx], p[indx], r[indx], vf[indx])
# apply the magnetic variation correction
ucor, vv_cor[indx, :] = magnetic_correction(theta[indx], uu, vv)
# scale northward velocity to m/s
vv_cor = vv_cor / 1000. # mm/s -> m/s
# return the Northward Velocity Profile
return vv_cor
