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Inversion Study of Vertical Eddy Viscosity Coefficient Based on an Internal Tidal Model with the Adjoint Method

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Based on an isopycnic-coordinate internal tidal model with the adjoint method, the inversion of spatially varying vertical eddy viscosity coefficient (VEVC) is studied in two groups of numerical experiments. In Group One, the influences of independent point schemes (IPSs) exerting on parameter inversion are discussed. Results demonstrate that the VEVCs can be inverted successfully with IPSs and the model has the best performance with the optimal IPSs. Using the optimal IPSs obtained in Group One, the inversions of VEVCs on two different Gaussian bottom topographies are carried out in Group Two. In addition, performances of two optimization methods of which one is the limited-memory Broyden-Fletcher-Goldfarb-Shanno (L-BFGS) method and the other is a simplified gradient descent method (GDM-S) are also investigated. Results of the experiments indicate that this adjoint model is capable to invert the VEVC with spatially distribution, no matter which optimization method is taken. The L-BFGS method has a better performance in terms of the convergence rate and the inversion results. In general, the L-BFGS method is a more effective and efficient optimization method than the GDM-S.
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Research Article
Inversion Study of Vertical Eddy Viscosity Coefficient Based on
an Internal Tidal Model with the Adjoint Method
Guangzhen Jin,1Qiang Liu,2and Xianqing Lv1
1Laboratory of Physical Oceanography, Ocean University of China, Qingdao 266100, China
2College of Engineering, Ocean University of China, Qingdao 266100, China
Correspondence should be addressed to Xianqing Lv; xqinglv@ouc.edu.cn
Received  March ; Revised  August ; Accepted  August 
Academic Editor: Fatih Yaman
Copyright ©  Guangzhen Jin et al. is is an open access article distributed under the Creative Commons Attribution License,
which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Based on an isopycnic-coordinate internal tidal model with the adjoint method, the inversion of spatially varying vertical eddy
viscosity coecient (VEVC) is studied in two groups of numerical experiments. In Group One, the inuences of independent point
schemes (IPSs) exerting on parameter inversion are discussed. Results demonstrate that the VEVCs can be inverted successfully
with IPSs and the model has the best performance with the optimal IPSs. Using the optimal IPSs obtained in Group One, the
inversions of VEVCs on two dierent Gaussian bottom topographies are carried outin Group Two.In addition, performances of two
optimization methods of which one is the limited-memory Broyden-Fletcher-Goldfarb-Shanno (L-BFGS) method and the other is
a simplied gradient descent method (GDM-S) are also investigated. Results of the experiments indicate that this adjoint model is
capable to invert the VEVC with spatially distribution, no matter which optimization method is taken. e L-BFGS method has a
better performance in terms of the convergence rate and the inversion results. In general, the L-BFGS method is a more eective
and ecient optimization method than the GDM-S.
1. Introduction
Internal tide, which is the internal wave of tidal frequency,
is a ubiquitous phenomenon in the oceans. Rattray [],
Baines [], Bell [], Baines [], Craig [], Gerkema [], and
Llewellyn Smith and Young [] have developed theoretical
models and obtained some analytical solutions of internal
tide on ideal topographies. ese theoretical models helped
them investigate the generation and propagation of inter-
nal tide. Although great progress has been made on the
internal tide theory and some analytical works were carried
out, only a small amount of solutions can be provided,
due to the complexity of the problems. For this reason,
quantitative analysis with practical signicance still has to
rely on the combination of numerical simulation, theoretical
analysis, experiment, and observation. Numerical simulation
is an eective method in marine research and has been
widely used in the internal tide research. Kang et al. []
investigated the 2internal tide near Hawaii with a two-
dimensional, two-layered numerical model and conrmed
that the internal tide was generated by barotropic forcing
at the Hawaiian Ridge and propagated in north-northeast
and south-southwest directions. Based on a high-precision
three-dimensional Princeton Ocean Model (POM), Niwa and
Hibiya [] obtained the distribution of the 2internal tide in
the Pacic Ocean using the TOPEX/Poseidon (T/P) satellite
data. Cummins et al. [] simulated the generation and
propagation of internal tides near the Aleutian Ridge using
T/P altimeter data. e comparison between the altimeter
data and their model results showed good agreement for the
phase, which also provided evidence for wave fraction near
theAleutianRidge.Withathree-dimensionalPOM,Niwa
and Hibiya [] investigated the distribution and the energy
of the 2internal tide around the continental shelf edge
in the East China Sea. eir numerical experiment results
indicated that 2internal tides are eectively generated over
prominent topographies such as sea ridges, island chains,
and straits. Jan et al. []modiedthePOMtostudythe
generation of the 1internal tide and its inuence on
surfacetideintheSouthChinaSea.econversionfrom
Hindawi Publishing Corporation
Mathematical Problems in Engineering
Volume 2015, Article ID 915793, 14 pages
http://dx.doi.org/10.1155/2015/915793
Mathematical Problems in Engineering
the barotropic energy to the baroclinic energy over topo-
graphicridgesintheLuzonStraitwasalsoestimated.
Determination of the vertical eddy viscosity coecient
(VEVC), which describes the vertical mixing in the ocean,
plays an important role in the study of energy exchange and
material transportation. e VEVC is regularly regarded as
a constant in numerical models. Schemes to determine the
VEVC mainly include the Prandtl mixing-length hypothesis
model, the -model, the Pacanowski-Philander mixing
model [], and some turbulent closure models that are
more complicated. Many studies have been carried out to
investigate the variation of the VEVC []. All these
mentioned studies indicate that due to dierent intensions
of the vertical mixing in sea water, the VEVC should
not be treated as a constant but a parameter with spatial
distribution.
Satelliteremotesensingtechnologyandotherrelated
technologiesprovideuswithalargenumberofdata.us,itis
one of the most important missions in physical oceanography
to make use of the data eciently and precisely as well
as to combine the observation data with present numerical
models. Indeed, data assimilation with the adjoint method
provides an eective access to these missions. e use of the
adjoint method in marine science can be traced back to s.
e adjoint model is capable of optimizing control param-
eters in numerical simulation. Bennett and McIntosh []
applied the weak constraint thought to solve the tidal problem
andthegeostrophic-owproblem.YuandOBrien[]
assimilated both meterological and oceanographic data into
an oceanic Ekman layer model and deduced the unknown
boundary condition, the unknown vertical eddy viscosity,
and the current eld. Based on a tidal model with a two-level
leapfrog method, Lardner [] inverted the open boundary
conditions in three-test problems. Seiler [] used the adjoint
method to assimilate observations into a quasi-geostrophic
ocean model and estimated the lateral boundary values in
ideal experiments. Navon []wroteasummaryofthe
parameter estimation in meteorology and oceanography in
the view of applications with four- dimensional variational
data assimilation techniques. Using an automatic dieren-
tiation compiler, Ayoub [] constructed the adjoint model
oftheMassachusettsInstituteofTechnologyOceanGeneral
CirculationModelandinvertedtheopenboundarycondi-
tions in the North Atlantic. Zhang and Lu []developed
a three-dimensional nonlinear numerical tidal model with
the adjoint method and designed several numerical exper-
iments to estimate three kinds of parameters including the
open boundary conditions, the bottom friction coecients,
and the vertical eddy viscosity coecients. Zhang and Lu
[] employed a two-dimensional tidal model to study the
inversion of the bottom friction coecients in the Bohai Sea
and the Yellow Sea with the adjoint method. Chen et al. []
constructed a three-dimensional internal tidal model with
theadjointmethodandestimatedsixdierentkindsofopen
boundary conditions on fourteen types of topography. Based
on a tidal model, Zhang and Chen [] carried out several
semiidealized experiments to estimate the partly and fully
spatial varying open boundary conditions. Cao et al. []
investigated the inversion of open boundary conditions with
a three-dimensional internal tidal model and simulated the
2internal tide around Hawaii by assimilating T/P data.
ere are two main objectives of this paper. One is to
study the inversion of the VEVC with an internal tidal model
and the adjoint method. According to the introductions
above, a lot of studies have been carried out to investigate the
inversion of the control parameters of internal tide such as
the open boundary condition [,]andthebottomfriction
condition [,]. However, few works are found to study
the inversion of VEVC. Since VEVC is a decisive factor to
describe the vertical mixing in the ocean, it is necessary to pay
attention to the inversion of the VEVC. e other objective is
to make a computational investigation on the performance
of the gradient descent method and the limited-memory
Broyden-Fletcher-Goldfarb-Shanno (L-BFGS) method for
the inversion of VEVCs based on the model constructed by
Chen et al. []. Both of the methods do not require any
evaluations of the Hessian matrices but gradient vectors and,
thus, are computationally feasible. Chen et al. [] have made
a comparative study on several optimization methods but it
is on the inversion of the open boundary conditions which
is a one-dimension case. e feasibility of these optimization
methods for two-dimensional case such as the inversion of
the VEVC needs further studies.
Two groups of numerical experiments are carried out
to study the inversion of spatially varying VEVCs based
on an isopycnic-coordinate internal tidal model with the
adjoint method. In Group One, the inuences of independent
point schemes (IPSs) exerting on parameter inversion are
discussed. Group Two investigates the inversions of VEVCs
on two dierent Gaussian bottom topographies and the
performances of two optimization methods which are the
GDM-S and the L-BFGS methods.
is paper is organized as follows. Section briey
introduces the adjoint tidal model and the methodology.
Two optimization methods, including the GDM-S and the L-
BFGS methods, are described in Section .Section presents
design and process of the experiments in detail. Results of
the experiments are discussed in Section . Finally, we make
a summary and draw some conclusions in Section .
2. Numerical Model Introduction
An isopycnic-coordinate internal tidal model with adjoint
assimilation method is employed in this paper. ere are two
parts in the internal tide model. One is forward model with
the governing equations and the other is adjoint model with
the adjoint equations. e two models are used to simulate
the internal tide and to optimize the control variables,
respectively. Chen et al. [] had introduced the two parts in
great detail and tested the reasonability and feasibility of the
model. e formulation will not be presented in this paper.
e derivation of VEVC adjustment, introduction of the two
optimization method, test of the adjoint method, and the
independent point scheme (IPS) are described in details in
this part.
Mathematical Problems in Engineering
2.1. Test of the Adjoint Method. According to the equations
and derivations of Chen et al. [], the formula to invert
the VEVC can be derived. e rst derivative of Lagrangian
function with respect to VEVC is obtained as follows:

V𝑖,𝑗,𝑘 =0, ()
where V𝑖,𝑗,𝑘 is the value of VEVC at grid (,)in the th layer.
e gradient of cost functions with respect to the VEVC in the
grid (,,)can be deduced as follows:

V𝑖,𝑗,𝑘
=𝑘+𝑘+1
×
𝑛
𝑛
𝑖,𝑗,𝑘 −𝑛
𝑖,𝑗,𝑘+1𝑛
𝑎𝑖,𝑗,𝑘 −𝑛
𝑎𝑖,𝑗,𝑘+1
𝑖,𝑗,𝑘 +𝑖+1,𝑗,𝑘 +𝑖,𝑗,𝑘+1 +𝑖+1,𝑗,𝑘+1
+𝑛
𝑖−1,𝑗,𝑘 −𝑛
𝑖−1,𝑗,𝑘+1𝑛
𝑎𝑖−1,𝑗,𝑘 −𝑛
𝑎𝑖−1,𝑗,𝑘+1
𝑖−1,𝑗,𝑘 +𝑖,𝑗,𝑘 +𝑖−1,𝑗,𝑘+1 +𝑖,𝑗,𝑘+1
+𝑘+𝑘+1
×
𝑛
V𝑛
𝑖,𝑗,𝑘 V𝑛
𝑖,𝑗,𝑘+1V𝑛
𝑎𝑖,𝑗,𝑘 V𝑛
𝑎𝑖,𝑗,𝑘+1
𝑖,𝑗,𝑘 +𝑖+1,𝑗,𝑘 +𝑖,𝑗,𝑘+1 +𝑖+1,𝑗,𝑘+1
+V𝑛
𝑖−1,𝑗,𝑘 V𝑛
𝑖−1,𝑗,𝑘+1V𝑛
𝑎𝑖−1,𝑗,𝑘 V𝑛
𝑎𝑖−1,𝑗,𝑘+1
𝑖−1,𝑗,𝑘 +𝑖,𝑗,𝑘 +𝑖−1,𝑗,𝑘+1 +𝑖,𝑗,𝑘+1
,
()
where 𝑘is the potential density in the th layer, 𝑛
𝑖,𝑗,𝑘 and
V𝑛
𝑖,𝑗,𝑘 are horizontal velocities at the th time step, 𝑛
𝑎𝑖,𝑗,𝑘 and
V𝑛
𝑎𝑖,𝑗,𝑘 are the adjoint variables of 𝑛
𝑖,𝑗,𝑘 and V𝑛
𝑖,𝑗,𝑘,respectively,
and 𝑖,𝑗,𝑘 is the initial thickness of the th layer. e detailed
derivation of () is presented in the appendix.
Accurately programming the adjoint in such problems as
the present one is quite tricky and experience has shown that
it is essential to check the accuracy of the adjoint computation
beforeproceedingwiththeminimizationruns[]. e
correctness of the adjoint method is veried in this section.
Take the rst-order term of a Taylor expansion for the cost
function and we obtain the following equation:
(p+U)=(p)+U⋅(p)+2. ()
Here, pis a general point of the control variable, (p)=
∇(p)isthecomputedgradient,andUis an arbitrary unit
vector in the parameter space. Based on () a function of
canbewrittenasfollows:
Φ()=(p+U)−(p)
U⋅(p),()
where is a small real number that is not equal to zero.
If the adjoint methodology is correct, it is supposed that
lim𝛼→0Φ() = 1according to (). In this paper, the VEVC
variable Vis treated as pand test of the adjoint method is
based on ().
In order to test the accuracy of the adjoint method, two
experiments are carried out in which two dierent types of U
are used. e dierent vector directions are 1=()/|()|
and 2=(1/,1/,...,1/),respectively.
Figure indicates the trends of Φ()as approaches to .
It is clear that in both experiments when is less than −3,
values of Φ(solidlines)arebothverycloseto(dashedlines).
Equation lim𝛼→0Φ() = 1is proved and the correctness of
gradient computed in the adjoint model is veried.
2.2. Independent Point Scheme. e available observation
data may not be sucient and control parameters to be
determined may be excessive in practice. at may cause
ill-posedness of the inversion problem. Richardson and
Panchang [] rst noted that if an adjoint method is applied,
when there is a big error in data, the solution will be unstable
and not unique. Many researchers have made progress in
solving this problem. A lot of work [,,,]havebeen
done to prove the capability and feasibility of the independent
point scheme (IPS) in solving ill-posed problems of inversion.
In this paper, the IPS is used to optimize the control
parameter. e basic idea of IPS is as follows: some grids (e.g.,
(,)) are selected as the independent points; it is assumed
that 𝑖𝑖,𝑗𝑗 represents the value of VEVC in grid (,),so
values of VEVC in all grids 𝑖,𝑗 can be calculated from 𝑖𝑖,𝑗𝑗
with linear interpolation method. e computing formula is
given as follows:
𝑖,𝑗 =𝑖𝑖,𝑗𝑗 𝑖,𝑗,𝑖𝑖,𝑗𝑗𝑖𝑖,𝑗𝑗
𝑖𝑖,𝑗𝑗 𝑖,𝑗,𝑖𝑖,𝑗𝑗 ,()
where 𝑖,𝑗,𝑖𝑖,𝑗𝑗 is the weight coecient of the Cressman form
[]:
𝑖,𝑗,𝑖𝑖,𝑗𝑗 =2−2
𝑖,𝑗,𝑖𝑖,𝑗𝑗
2+2
𝑖,𝑗,𝑖𝑖,𝑗𝑗 ,()
where 𝑖,𝑗,𝑖𝑖,𝑗𝑗 is the center distance between (,)and (,)
and is the inuence radius. According to (), the gradient
of with respect to 𝑖,𝑗 canbewrittenas

𝑖𝑖,𝑗𝑗 =
𝑖,𝑗 𝑖,𝑗,𝑖𝑖,𝑗𝑗 
𝑖,𝑗
𝑖,𝑗 𝑖,𝑗,𝑖𝑖,𝑗𝑗,()
where /𝑖,𝑗 is the gradient of with respect to the VEVC
at the grid (,)and can be calculated using formula ().
According to Section ., the correctness of the gra-
dient with respect to the independent points should be
tested. Based on (), the perturbations ()applied to the
independent points have a linear impact on those applied
to the nonindependent points. e convergences for the
nonindependent points will remain the same aer linear
transformation for independent points.
e values of VEVC at the independent grids can be
calculated inside the model and values at other grids are
Mathematical Problems in Engineering
−5
−4−3−2−10
−0.5
0
0.5
1
1.5
2
2.5
log10Φ(𝛼 )
log10𝛼
U1
(a)
1
0.8
0.6
0.4
0.2
0
−0.2
U2
−5
−4−3−2−10
log10Φ(𝛼 )
log10𝛼
(b)
F : Variation of Φ()with respect to .
gained through interpolation using (). en the spatial
distribution of VEVC in the entire area is obtained.
3. Optimization Algorithms
ere have been many large-scale optimization methods to
solve the minimization problem []. Four main methods
arelinesearchmethod(e.g.,WolfeandGoldstein),trust-
region method, conjugate gradient method (e.g., Fletcher-
Reeves), and quasi-newton method (e.g., BFGS and L-BFGS).
However, the number of studies discussing the performances
of various optimization methods in the meteorological and
oceanographic application is still relatively small []. Line
search method requires repeated computations for the cost
function and the gradient. erefore it spends too much com-
putation resource during numerical simulations especially for
physical oceanography. Besides, line search methods may fail
in some cases []. e L-BFGS method is commonly used to
solve large-scale problems in oceanography and meteorology
[,,]. Chen et al. [] have made a computational
investigation on the performances of the L-BFGS method and
two versions of gradient descent method with an internal tide
model. In their work, a simplied gradient descent method
is applied which is able to avoid too much computation.
e step length is chosen according to the experience of the
modeler. Compared with other methods, there are two main
advantages of this plan. One is the less computation resource
usage and the other is the more controllable optimization
process. Many research papers have proved the feasibility of
this method [,,].
Generally speaking, numerical methods to solve the
minimization problems have the similar iterative formula as
follows:
𝑛+1
V=𝑛
V+𝑛𝑛,()
where 𝑛
Vand 𝑛+1
Vare the priori and adjusted values of
VEVC in the th iteration, respectively and 𝑛and 𝑛
represent the iteration step length and the search direction,
respectively. ere are many methods to determine the search
direction 𝑛. Two dierent optimization methods employed
in this paper are the GDM-S and the L-BFGS methods.
3.1. Gradient Descent Method (GDM). e GDM is a simple
and feasible method to dene the search direction as follows:
𝑛=−𝑛=−/V𝑖,𝑗,𝑘𝑛
/V𝑖,𝑗,𝑘𝑛
,()
where ,,andare the zonal index, the meridional index,
and the layer index of the calculation grid, respectively;
represents the step of iteration. (/V𝑖,𝑗,𝑘)𝑛is the 2norm
of the gradient of the cost function with respect to the VEVC
in the th iteration.
In the GDM-S, the step length is chosen to be a constant
according to the experience of the modeler. We have surveyed
the performances of dierent values of andtake.asthe
best choice. e optimized value of VEVC is obtained aer
the VEVC in every grid (,,) is adjusted according to ()
and ().
3.2. L-BFGS Method. L-BFGS is an optimization algorithm
in the family of quasi-Newton methods that approximates the
BFGS algorithm using a limited amount of computer mem-
ory. is method is rst described in the work of Nocedal
[],whereitiscalledtheSQNmethod.Itisapopular
algorithm for parameter estimation in machine learning [,
]. Due to its resulting linear memory requirement, the
L-BFGS method is particularly well suited for optimization
problems with a large number of variables.
It requires the search direction to be
𝑘=−𝑘𝑘,()
Mathematical Problems in Engineering
where
𝑘+1 =
𝑇
𝑘−1 ⋅⋅⋅𝑇
𝑘−𝑚0𝑘−𝑚 ⋅⋅⋅𝑘−1
+𝑘−𝑚 𝑇
𝑘⋅⋅⋅𝑇
𝑘−𝑚+1𝑘−𝑚𝑇
𝑘−𝑚 𝑘−𝑚+1 ⋅⋅⋅𝑘
+𝑘−𝑚 𝑇
𝑘⋅⋅⋅𝑇
𝑘−𝑚+1𝑘−𝑚𝑇
𝑘−𝑚 𝑘−𝑚+1 ⋅⋅⋅𝑘
+𝑘−𝑚 𝑇
𝑘⋅⋅⋅𝑇
𝑘−𝑚+1𝑘−𝑚𝑇
𝑘−𝑚 𝑘−𝑚+1 ⋅⋅⋅𝑘
...
+𝑘𝑘𝑇
𝑘.()
Note that 𝑘is the simplication of ∇(𝑘)for conve-
nience. Here, 𝑘=1/𝑘𝑇
𝑘,𝑘=1−𝑘𝑘𝑇
𝑘,𝑘=𝑘+1 −𝑘=
𝑘𝑘,and𝑘=
𝑘+1 −
𝑘. Many studies have shown that
typically 3≤≤7,where>7does not improve the
performanceofL-BFGS[]. So the number of corrections
m used in the L-BFGS update of this paper is taken as [].
e version of L-BFGS used in this paper is described in Liu
and Nocedal [] and the Fortran codes are authorized by
Nocedal [].
4. Design of Experiments
All the experiments in this paper are implemented in an ideal
regional area from Eto.
Eandfrom
N to .N
with in mind the practical sea area located around the Luzon
strait. e horizontal resolution is 10󸀠×10󸀠and there are
totally 49×31grids in the area. e maximum depth is set
to be  meters. e horizontal eddy coecient is chosen
to be =1000and the bottom friction coecient is taken
as = 0.003. e Coriolis coecient is taken as the local
value. Only 2tide is considered and its angular frequency is
1.41×10−4 s−1. e whole-time step is . s which is /
of the period of 2tide. All the four boundaries are open
boundaries and boundary conditions are set to be the local
water levels in the Flather form.
Eastern and western boundaries:
−
󸀠1 2
2

, ()
positive in eastern boundary and negative in western bound-
ary.
North and south boundaries:
−
󸀠1 2
2

, ()
positive in north boundary and negative in south boundary.
is the surface elevation above the undisturbed sea level.
and are the zonal current velocity and the meridional
current velocity, respectively.
󸀠,
,and
are the surface
elevation and the zonal and meridional current velocity
relating to the boundary barotropic tidal force, respectively.
is the Coriolis coecient and is the tidal frequency of 2
tide. is the local water depth and is the acceleration of
gravity.
Similar as Chen et al. [], the 2tidal force at the th
time step is subject to
󸀠2 =𝜁cos ()+𝜁sin (),()
the Fourier coecients 𝜁at four open boundaries are set to
be and 𝜁are set to be () at the north and west (south
and east) boundaries.
e T/P altimeter data is widely spread throughout the
oceananditcanbeusedtoinvertVEVC.Inthiswork,wepick
 calculating points based on the distribution features of T/P
altimeter observation as the observation points (Figure ).
Two kinds of topographies are tested in this paper and
they are generated based on the two formulas in (),
respectively (Figure ). e sea water in the computing area
is divided into two layers. e thicknesses of each layers are,
respectively, 1= 200mand2= 800m. e potential
densities of corresponding layer are 1=1021(kg/m−3)and
2=1024(kg/m−3), respectively. Consider
𝐴=0exp −02+−02
22
MaxDepth,
𝐵=01exp −−02+−02
22
MaxDepth,
()
where 0istheheightofthetopographyandMaxDepthisthe
depth of the water.
For each experiment, the optimization of the VEVC can
be implemented with the following steps.
Step 1. e prescribed VEVC is given and the forward model
is run. e whole simulation time is  period of the 2
tide in order to obtain a stable simulation result. e water
elevations in the observation positions are treated as the
“pseudoobservations.”
Step 2. Initial value of the control parameter (VEVC) is given
and forward model is run to get the simulated results of all the
state variables such as current velocity and water elevation.
e value of cost function is calculated.
Step 3. Dierence between the simulated elevation and the
“pseudoobservation” plays as the external force of the adjoint
model. Via backward integrating the adjoint equations in
aperiodofthe2tide values of the adjoint variables are
obtained.
Step 4. Using formula (), along with the state variables and
the adjoint variables obtained in Steps and ,thegradient
of cost function with respect to VEVC is calculated.
Mathematical Problems in Engineering
116.5 117 117.5 118 118.5 119 119.5 120 120.5
18.5
19
19.5
20
20.5
21
−1000
−950
−900
−850
−800
−750
−700
−650
−600
−550
−500
Latitude (N)
Longitude (E)
F : Planform of topography (e.g., topography A) and loca-
tions of the observations (white dots).
Step 5. Update the unknown control variables with a certain
optimization method.
Step 6. If the stopping criterion of iteration is reached, bring
the iteration to an end and return the optimized parameter.
Otherwise, update all the parameters and go back to Step .
In the experiments of this paper, all initial values of VEVC
are set to . and the total number of iterations is allowed
to be  at most. e chosen convergence criterion is that
the last two values of the cost function are suciently close,
which is dened by end −end−1<10−9,()
where end and end−1 are the last and the second last values of
the cost function, respectively.
Two groups of numerical experiments are carried out:
theinuenceofIPSsontheinversionofVEVCisstudied
inGroupOne;inGroupTwotheabilityofthisinternal
tide model to invert dierent kinds of VEVC with spatial
distribution is examined. Two kinds of spatial distribution
ofVEVCareprescribedandgiveninFigure .Forboth
distributions, the VEVC value ranges from 3×10−3 m2/s to
7×10−3 m2/s.
In Group One, nine experiments are carried out to discuss
the inuence of IPS on the inversion of VEVC. e distance
between independent points (IP) ranges from 󸀠(length of
grids)to
󸀠(length of  grids) and details are listed
in Table . Topography A is applied and distribution (a) is
chosen to be the prescribed spatial distribution of VEVC.
In Group Two, four numerical experiments (NEs) are
carriedoutwhicharenumberedasNENE, respectively.
Each experiment is implemented with GDM-S and the L-
BFGS methods. Information of topographies and prescribed
VEVCs for all NEs is listed in Table .eIPSsarethe
optimal schemes obtained in Group One. Other parameters
are exactly the same as Group One.
All the experiments in Group One and Group Two are
carried out following Steps to described in Section .
VersionofL-BFGSmethodusedinthispaperisfromthe
work of Liu and Nocedal [].
T : Settings of independent point schemes in Group One.
IPS
NumberofIPs 
Distance between IPs (󸀠) 
T : Topographies and distributions of VEVC in Group Two.
Experiment Topography Distribution
NE A a
NE A b
NE B a
NE B b
5. Experiment Results and Discussions
5.1. Results and Discussions of Group One. Figure illustrates
therelationshipsbetweenmeanabsoluteerrors(MAE,which
reects the error between the inversion result and the given
VEVC) and the distance between independent points in
Group One.
As is shown in Figure , MAEs with dierent optimiza-
tion methods vary as the IPSs change. e minimum MAEs
with the two methods are not the same (dashed lines). e
minimum MAE with the GDM-S is 2.66× 10−4 m2/s while
that with the L-BFGS method reaches 9.14×10−5 m2/s. e
corresponding IP distances are 󸀠(length of grids, GDM-
S) and 󸀠(lengthofgrids,L-BFGS),respectively.According
to the MAEs illustrated in Figure , the optimal IPSs of the
two methods are selected as IPS (GDM-S) and IPS (L-
BFGS).
5.2. Results and Discussions of Group Two. With the respec-
tive optimal IPSs and the iteration process in Section ,the
VEVCs are inverted with GDM-S method (I) and L-BFGS
method (II), respectively, and the inversion results are shown
in Figure .
Comparison of the inversion results with the prescribed
VEVCs indicates that all the given spatial distributions of
VEVC are successfully inverted aer  iteration steps. e
main features of all distributions can be recovered very well.
Surfaces of the inverted VEVC with the L-BFGS are much
smoother than those with the GDM-S. Compared against
the inversion results with the GDM-S (le panels), patterns
with the L-BFGS method (right panels) are closer to the
prescribed VEVC. More statistic data will be presented in the
next paragraphs.
MAEs of the four numerical experiments aer assimila-
tion are calculated and listed in Table .einitialvaluesof
MAE in all NEs are 1×10−3 m2/s. Based on the results shown
in Table , all the MAEs aer assimilation are more than one
order of magnitude lower than the initial values, which means
the success for both of the two optimization methods. Note
that the MAEs with the L-BFGS method are quite close (less
than 1×10−8 m2/s and cannot be distinguished in the table)
and are less than half of those with the GDM-S. is result
demonstrates the ability of the L-BFGS method to deduce the
overall errors.
Mathematical Problems in Engineering
10
20 30
40
10
20
30
−1000
−800
−600
−400
−200
0
Zonal index
Meridional index
A
(a)
10
B
20
30 40
10
20
30
−1000
−800
−600
−400
−200
0
Zonal index
Meridional index
10
2
0
30
40
10
20
Zon
al
index
idi
al
(b)
F : Topographies A and B. Note that the abscissa and ordinate axes are labeled with zonal index and meridional index, respectively.
116.5 117 117.5 118 118.5 119 119.5 120 120.5
18.5
19
19.5
20
20.5
21
3
3.5
4
4.5
5
5.5
6
6.5
7
×10−3
Latitude (N)
Longitude (E)
(a)
116.5 117 117.5 118 118.5 119 119.5 120 120.5
18.5
19
19.5
20
20.5
21
3
3.5
4
4.5
5
5.5
6
6.5
7
×10−3
Latitude (N)
Longitude (E)
(b)
F : Planform of two prescribed spatial distributions of VEVC.
T : Inversion errors of VEVC in Group Two (unit: m/s).
Method Experiment
NE NE NE NE
GDM-S(I) 2.4204 2.4304 2.2304 2.2404
L-BFGS(II) 9.1405 9.1405 9.1405 9.1405
To compare the eectiveness of the two methods to invert
the VEVC, we make statistics on the percentages of the grids
20 30 40 50 60 70 80 90 100
0
0.5
1
1.5
2
2.5
3
×10−3
MAE (m2/s)
IP distance
GDM-S
L-BFGS
F : MAEs versus IP distance in Group One. e abscissas
indicates distance between adjacent IPs (unit: 󸀠) while the ordinate
indicates MAE of inversion results. e solid lines are values of
dierent experiments and the dashed lines indicate the minimum
values of two solid lines, respectively.
at which the MAEs are less than 1×10
−4 m2/s, which is
listed in Tabl e . With the GDM-S, the inversion errors are
deduced by one order of magnitude at about % of the
total grids. By contrast, ratios of all NEs with the L-BFGS
method are .%, without dierences between NEs. is
phenomenon indicates that the L-BFGS method is eective at
more computation grids than the GDM-S. Furthermore, the
L-BFGS method maintains its eectiveness no matter which
topography is applied.
Combining the inversion patterns, the inversion errors of
the VEVC, and the eectiveness analyses, conclusions can be
drawn that the L-BFGS has a better performance in reducing
the inversion errors.
Finally we come to the optimization history for all the
experiments carried out in Group Two. e variations of the
cost function normalized by its initial value, that of the 2
norm of the gradient of the cost function with respect to the
Mathematical Problems in Engineering
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(a) NE(I)
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(b) NE(II)
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(c) NE(I)
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(d) NE(II)
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(e) NE(I)
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(f) NE(II)
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(g) NE(I)
117 118 119 120
19
20
21
Latitude (N)
Longitude (E)
(h) NE(II)
F : Planform of inversion results in Group Two.
Mathematical Problems in Engineering
T : Eectiveness analyses of inversions in Group Two.
Method Experiment
NE NE NE NE
GDM-S(I) .% .% .% .%
L-BFGS(II) .% .% .% .%
VEVCs and that of the inversion error, are plotted in Figures
(a),(b),and(c), respectively, as a function of the iteration
step.
Note that all experiments with the L-BFGS method reach
the convergence criterion and stop aer iterations, which
indicates that the computation time for the L-BFGS method is
one twenty-h of that for the GDM-S. Figure (a) indicates
that all the cost functions are in downward trends throughout
the iteration process and decrease by more than () orders of
magnitude for the GDM-S (L-BFGS method), which means
that the nal dierences between simulation value and the
observation of these two methods are less than one-tenth
and one-thousandth of their initial values, respectively. As is
shown in Figure (b),the2norms of gradient of the cost
function with respect to the VEVC decrease by more than
order of magnitude (GDM-S) and orders of magnitude
(L-BFGS), compared with their respective initial values. is
indicates that the inversion result is becoming increasingly
closer to the given VEVC during the iteration. As shown
in Figure (c), the inversion errors with the two methods
keep declining throughout the iterations until the stopping
criterions are satised. In general, the cost functions, norms
of gradient, and the inversion errors of the VEVC have
steady descent, which demonstrates that this adjoint model
is capable to invert the VEVC. What is more, both the
GDM-SandtheL-BFGSmethodsareeectiveinterms
of the inversion of the control parameters with spatially
distributions of internal tide.
It is also clear in Figure that the convergence rate for the
cost functions, norms of gradient, and the inversion errors
of the VEVC is much faster with the L-BFGS method than
those with the GDM-S, which is consistent with the classic
theories about the convergence rate of the quasi-Newton
method and the GDM []. is trend is also consistent
with the results of numerical experiments to invert the open
boundary conditions in Chen et al. []. With no doubt, the
L-BFGS method is a more eective and ecient optimization
method to invert the spatially varying VEVC. However, the
GDM-S is easier to understand and to implement in the
model. Moreover, the step length and the search direction
in the process of GDM-S can be freely controlled by the
modelers, which is very convenient in practice. erefore,
for the inversion of the VEVC, the GDM-S should also be
regarded as a choice.
6. Summary and Conclusions
Based on an isopycnic-coordinate internal tidal model, the
inversion of VEVC is studied in this paper. A series of
numerical experiments are carried out to examine the inu-
ence factors on the inversion of VEVCs in four aspects:
independent point schemes (IPS), topography, the spatial
distribution of VEVC, and the optimization methods. For
each experiment, the cost function, the 2norm of gradient
of cost function with respect to the VEVC, and the inversion
errorarecalculatedandanalyzedindetails.
e IPS is introduced and discussed in Group One. All
the VEVCs can be inverted successfully with IPS. MAE is
regarded as the comparison criterion of the result. Aer
comparing the experiments, the correctness of the IPS is
conrmed and the optimal IPSs are selected for the GDM-S
and the L-BFGS methods, respectively.
BasedontheoptimalIPSsinGroupOne,twokindsof
VEVC distributions are successfully inverted with this adjoint
model on two kinds of topography in Group Two. MAEs aer
optimization are at the level of −4 (−5)fortheGDM-S
(L-BFGS), which is one (two) order(s) of magnitude lower
than the initial value. All the cost functions and their gradient
norms with respect to the VEV lead satisfactory declines no
matter which optimization method is taken. Compared with
the GDM-S, the L-BFGS method has a remarkably better
performance, not only in terms of the convergence rate but
also in terms of the nal inversion results. e computation
time for the L-BFGS method is much shorter than that for
theGDM-S.Tosumup,theL-BFGSmethodisamore
eective and ecient method than the GDM-S in terms of
the inversion of the VEVC. Nevertheless, the GDM-S is more
convenientandcontrollablesoitshouldnotbeignoredand
should be taken seriously as a choice for the inversion of the
VEVC with spatially distribution.
e success of numerical experiments lays a solid founda-
tion for the practical experiments and encourages us to carry
out experiments in practical sea area with measured data and
the real T/P altimeter data.
Appendix
Derivation of ()
Let us start with the governing equations in Chen et al. [].
Layer (surface layer)
1
 +1
cos 11
 +1
cos 1V1cos 
 =0,
(A.a)
1
 +1
cos 1
 +V1
1
 1V1tan
−V1−ℎ11
+1𝜆
1+
cos
 𝑙
𝑚=1 𝑚
𝑚−𝑚+1
𝑘
=0,
(A.b)
V1
 +1
cos V1
 +V1
V1
 +2
1tan
−1−ℎ1V1
+1𝜑
1+
 𝑙
𝑚=1 𝑚
𝑚−𝑚+1
𝑘
=0.
(A.c)
 Mathematical Problems in Engineering
−10
−5
0
log10(J/J0)
10 20 30 40 50 60 70 80 90 100
Iteration steps
(a)
10 20 30 40 50 60 70 80 90 100
Iteration steps
−4
−2
0
log10(G/G0)
(b)
NE1(I)
NE2(I)
NE3(I)
NE4(I)
NE1(II)
NE2(II)
NE3(II)
NE4(II)
10 20 30 40 50 60 70 80 90 100
Iteration steps
−4
−3.5
−3
log10(MAE)
(c)
F : Optimization history for experiments of Group Two, about (a) the cost function normalized by its initial value 0,(b)the2norm
of gradient of the cost function with respect to the VEVC, and (c) the MAEs between the inverted and prescribed VEVCs.
Layer (=2,...,−1)
𝑘
 +1
cos 𝑘𝑘
 +1
cos 𝑘V𝑘cos 
 =0,
(A.a)
𝑘
 +𝑘
cos 𝑘
 +V𝑘
𝑘
 𝑘V𝑘tan
−V𝑘−ℎ𝑘𝑘
(𝑘−1)𝜆−𝑘𝜆
𝑘+
cos
×𝑘−1
𝑚=1 1
𝑘1
𝑚𝑚

+
 𝑙
𝑚=1 𝑚
𝑚−𝑚+1
𝑘
=0,
(A.b)
V𝑘
 +𝑘
cos V𝑘
 +V𝑘
V𝑘
 +2
𝑘tan
+𝑘
−ℎ𝑘V𝑘(𝑘−1)𝜑−𝑘𝜑
𝑘+
×𝑘−1
𝑚=1 1
𝑘1
𝑚𝑚

+
 𝑙
𝑚=1 𝑚
𝑚−𝑚+1
𝑘
=0.
(A.c)
Layer (bottom layer)
𝑙
 +1
cos 𝑙𝑙
 +1
cos 𝑙V𝑙cos 
 =0, (A.a)
𝑙
 +𝑙
cos 𝑙
 +V𝑙
𝑙
 𝑙V𝑙tan
−V𝑙
−ℎ𝑙𝑙(𝑙−1)𝜆−𝑏𝜆
𝑙+
cos
×
 𝑙
𝑚=1 𝑚
𝑙−𝑚+1
𝑙
=0,
(A.b)
V𝑙
 +𝑙
cos V𝑙
 +V𝑙
V𝑙
 +2
𝑙tan
+𝑙
−ℎ𝑙V𝑙(𝑙−1)𝜑−𝑏𝜑
𝑙+
×
 𝑙
𝑚=1 𝑚
𝑙−𝑚+1
𝑙
=0.
(A.c)
e variables and background of the governing equations
have been introduced in Chen’s [] work in details. We will
not repeat them in this part. e interface and friction terms
are expressed by
𝑘𝜆,𝑘𝜑=V𝑘𝑘+1/2
𝑘+1/2 𝑘−𝑘+1,V𝑘V𝑘+1,
=1,...,−1, (A.)
where Vis the vertical eddy viscosity coecient, 𝑘+1/2 =
(𝑘+𝑘+1)/2,and𝑘+1/2 =(𝑘+𝑘+1)/2.
Mathematical Problems in Engineering 
e cost function is dened as
,,V;p
=1
2
𝜍
𝑙
𝑘=1𝑙
𝑚=𝑘 𝑚
𝑚−𝑚
𝑘2
+𝑢
𝑙
𝑘=1𝑘
𝑘2+V
𝑙
𝑘=1V𝑘
V𝑘2
,
(A.)
which is exactly the same as that in []. en the Lagrangian
function is dened as
,,V;𝑎,𝑎,V𝑎;p
=,,V;p
+𝑎1 (A.1a)+𝑎11(A.1b)+V𝑎11(A.1c)
+⋅⋅
+𝑎𝑘 (A.2a)+𝑎𝑘𝑘(A.2b)+V𝑎𝑘𝑘(A.2c)
+⋅⋅
+𝑎𝑙 (A.3a)+𝑎𝑙𝑙(A.3b)+V𝑎𝑙𝑙(A.3c),
(A.)
where
(A.1a)
=−1
 +1
cos 11
 +1
cos 1V1cos 
 ,
(A.)
(A.1b)=−1
 +1
cos 1
 +V1
1
 1V1tan
−V1−ℎ11+1𝜆
1+
cos
×
 𝑙
𝑚=1 𝑚
𝑚−𝑚+1
𝑘
,
(A.)
(A.1c)=−V1
 +1
cos V1
 +V1
V1
 +2
1tan
−1−ℎ1V1+1𝜑
1+
×
 𝑙
𝑚=1 𝑚
𝑚−𝑚+1
𝑘
,
(A.)
samedenitionsareappliedin(A.a)(A.c)and(A.a)
(A.c). en the Lagrangian function (,,V;𝑎,𝑎,V𝑎;p)
can be written as
,,V;𝑎,𝑎,V𝑎;p
=,,V;p
𝑎1V𝑖+1/2,𝑗,11+1/2
𝑖+1/2,𝑗,1+1/2 1−2
+𝑎1V𝑖+1/2,𝑗,11+1/2
𝑖+1/2,𝑗,1+1/2 V1V2−1
+⋅⋅
𝑎𝑘V𝑖+1/2,𝑗,𝑘𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 𝑘−𝑘+1
𝑎𝑘V𝑖+1/2,𝑗,𝑘−1𝑘−1/2
𝑖+1/2,𝑗,𝑘−1/2 𝑘−1 −𝑘
V𝑎𝑘V𝑖+1/2,𝑗,𝑘𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 V𝑘−V𝑘+1
V𝑎𝑘V𝑖+1/2,𝑗,𝑘−1𝑘−1/2
𝑖+1/2,𝑗,𝑘−1/2 V𝑘−1 V𝑘−𝑘
+⋅⋅
+𝑎𝑙V𝑖+1/2,𝑗,𝑙−1𝑙−1/2
𝑖+1/2,𝑗,𝑙−1/2 𝑙−1 −𝑙
+𝑎𝑙V𝑖+1/2,𝑗,𝑙−1𝑙−1/2
𝑖+1/2,𝑗,𝑙−1/2 V𝑙−1 V𝑙−𝑙,
(A.)
where V𝑖+1/2,𝑗,𝑘 =(V𝑖,𝑗,𝑘V𝑖+1,𝑗,𝑘)/2,𝑖+1/2,𝑗,𝑘+1/2 =(
𝑖,𝑗,𝑘 +
𝑖+1,𝑗,𝑘 +𝑖,𝑗,𝑘+1 +𝑖+1,𝑗,𝑘+1)/4, and functions 1,𝑘,and𝑙are,
respectively, dened as
1=𝑎1 (A.1a)+𝑎11⋅(A.1b)+1𝜆
1
+V𝑎11⋅(A.1c)+1𝜑
1, (A.)
 Mathematical Problems in Engineering
𝑘=𝑎𝑘 (A.2a)+𝑎𝑘𝑘⋅(A.2b)(𝑘−1)𝜆 −𝑘𝜆
1
+V𝑎𝑘𝑘⋅(A.2c)(𝑘−1)𝜑 −𝑘𝜑
𝑘, (A.)
𝑙=𝑎𝑙 (A.3a)+𝑎𝑙𝑙⋅(A.3b)(𝑙−1)𝜆
𝑙
+V𝑎𝑙𝑙⋅(A.3c)(𝑙−1)𝜑
𝑙. (A.)
Note that (A.)(A.)donotcontainthevariableV,which
means 1
V𝑖,𝑗,𝑘 =𝑘
V𝑖,𝑗,𝑘 =𝑙
V𝑖,𝑗,𝑘 =0. (A.)
e Lagrangian function can be written as
,,V;𝑎,𝑎,V𝑎;p
=,,V;p
𝑎1,𝑗,1V𝑖+1/2,𝑗,11+1/2
𝑖+1/2,𝑗,1+1/2 𝑖,𝑗,1 −𝑖,𝑗,2
+𝑎1,𝑗,1V𝑖+1/2,𝑗,11+1/2
𝑖+1/2,𝑗,1+1/2 V𝑖,𝑗,1 V𝑖,𝑗,2−1
+⋅⋅
𝑎𝑖,𝑗,𝑘V𝑖+1/2,𝑗,𝑘𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 𝑖,𝑗,𝑘 −𝑖,𝑗,𝑘+1
𝑎𝑖,𝑗,𝑘V𝑖+1/2,𝑗,𝑘−1𝑘−1/2
𝑖+1/2,𝑗,𝑘−1/2 𝑖,𝑗,𝑘−1 −𝑖,𝑗,𝑘
V𝑎𝑖,𝑗,𝑘V𝑖+1/2,𝑗,𝑘𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 V𝑖,𝑗,𝑘 V𝑖,𝑗,𝑘+1
V𝑎𝑘V𝑖+1/2,𝑗,𝑘−1𝑘−1/2
𝑖+1/2,𝑗,𝑘−1/2 V𝑖,𝑗,𝑘−1 V𝑖,𝑗,𝑘−𝑘
+⋅⋅
+𝑎𝑖,𝑗,𝑙V𝑖+1/2,𝑗,𝑙−1𝑙−1/2
𝑖+1/2,𝑗,𝑙−1/2 𝑖,𝑗,𝑙−1 −𝑖,𝑗,𝑙
+𝑎𝑖,𝑗,𝑙V𝑖+1/2,𝑗,𝑙−1𝑙−1/2
𝑖+1/2,𝑗,𝑙−1/2 V𝑖,𝑗,𝑙−1 V𝑖,𝑗,𝑙−𝑙.
(A.)
Finally, according to the typical theory of Lagrangian
multiplier method, we have the following rst-order derivate
of Lagrangian function with respect to the control parameter
V:

V𝑖,𝑗,𝑘 =0, (A.)
then the gradient of the cost function with respect to the
variable Vcanbededucedfrom(A.):

V𝑖,𝑗,𝑘
=
𝑛𝑛
𝑎𝑖,𝑗,𝑘 𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 𝑛
𝑖,𝑗,𝑘 −𝑛
𝑖,𝑗,𝑘+1
+𝑛
𝑎𝑖−1,𝑗,𝑘 𝑘+1/2
𝑖−1/2,𝑗,𝑘+1/2 𝑛
𝑖−1,𝑗,𝑘 −𝑛
𝑖−1,𝑗,𝑘+1
𝑛𝑛
𝑎𝑖,𝑗,𝑘+1 𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 𝑛
𝑖,𝑗,𝑘 −𝑛
𝑖,𝑗,𝑘+1
+𝑛
𝑎𝑖−1,𝑗,𝑘+1 𝑘+1/2
𝑖−1/2,𝑗,𝑘+1/2 𝑛
𝑖−1,𝑗,𝑘 −𝑛
𝑖−1,𝑗,𝑘+1
+
𝑛V𝑛
𝑎𝑖,𝑗,𝑘 𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 V𝑛
𝑖,𝑗,𝑘 V𝑛
𝑖,𝑗,𝑘+1
+V𝑛
𝑎𝑖−1,𝑗,𝑘 𝑘+1/2
𝑖−1/2,𝑗,𝑘+1/2 V𝑛
𝑖−1,𝑗,𝑘 V𝑛
𝑖−1,𝑗,𝑘+1
𝑛V𝑛
𝑎𝑖,𝑗,𝑘+1 𝑘+1/2
𝑖+1/2,𝑗,𝑘+1/2 V𝑛
𝑖,𝑗,𝑘 V𝑛
𝑖,𝑗,𝑘+1
+V𝑛
𝑎𝑖−1,𝑗,𝑘+1 𝑘+1/2
𝑖−1/2,𝑗,𝑘+1/2 V𝑛
𝑖−1,𝑗,𝑘 V𝑛
𝑖−1,𝑗,𝑘+1
=𝑘+𝑘+1
×
𝑛
𝑛
𝑖,𝑗,𝑘 −𝑛
𝑖,𝑗,𝑘+1𝑛
𝑎𝑖,𝑗,𝑘 −𝑛
𝑎𝑖,𝑗,𝑘+1
𝑖,𝑗,𝑘 +𝑖+1,𝑗,𝑘 +𝑖,𝑗,𝑘+1 +𝑖+1,𝑗,𝑘+1
+𝑛
𝑖−1,𝑗,𝑘 −𝑛
𝑖−1,𝑗,𝑘+1𝑛
𝑎𝑖−1,𝑗,𝑘 −𝑛
𝑎𝑖−1,𝑗,𝑘+1
𝑖−1,𝑗,𝑘 +𝑖,𝑗,𝑘 +𝑖−1,𝑗,𝑘+1 +𝑖,𝑗,𝑘+1
+𝑘+𝑘+1
×
𝑛
V𝑛
𝑖,𝑗,𝑘 V𝑛
𝑖,𝑗,𝑘+1V𝑛
𝑎𝑖,𝑗,𝑘 V𝑛
𝑎𝑖,𝑗,𝑘+1
𝑖,𝑗,𝑘 +𝑖+1,𝑗,𝑘 +𝑖,𝑗,𝑘+1 +𝑖+1,𝑗,𝑘+1
+V𝑛
𝑖−1,𝑗,𝑘 V𝑛
𝑖−1,𝑗,𝑘+1V𝑛
𝑎𝑖−1,𝑗,𝑘 V𝑛
𝑎𝑖−1,𝑗,𝑘+1
𝑖−1,𝑗,𝑘 +𝑖,𝑗,𝑘 +𝑖−1,𝑗,𝑘+1 +𝑖,𝑗,𝑘+1
.
(A.)
Conflict of Interests
e authors declare that there is no conict of interests
regarding the publication of this paper.
Mathematical Problems in Engineering 
Acknowledgments
Partial support for this research was provided by the
National Natural Science Foundation of China through Grant
, the State Ministry of Science and Technology of
China through Grant AA, and the Fundamental
Research Funds for the Central Universities  and
.
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... (3) 以流速观测值和模拟值的差驱动反向模型, 对猜测值进行优化; [37][38][39] ; 不过, 也有研究认为 GD 法反演的结果 更好 [40][41] 可能导致对一部分地转流速与 Ekman 流速发生混叠, 造成对 Ekman 流速的错误估计 [52][53] 。为此, 我们参 考 Roach 等的做法, 将地转剪切也考虑进来, 把地转 流速拆分为两部分 [54] : ...
... coefficient (Zhang et al., 2015), and time-varying vertical eddy viscosity coefficients in oceanic Ekman layer models, and the spatially varying settling velocity (Zhang et al., 2018) in SSTMs. In several other studies, the CG (Alekseev et al., 2009;Navon and Legler, 1987) and L-BFGS methods (Jin et al., 2015;Zhang and Wang, 2014;Zou et al., 1993) had the best performance. Thus, they should be compared to select the best algorithm. ...
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In this paper, an improved numerical scheme is developed to estimate the initial conditions (ICs) based on a three-dimensional suspended sediment transport model (3D SSTM) with adjoint data assimilation, and the method is then applied to Hangzhou Bay as an example. Specifically, the ICs are estimated by assimilating artificial observations in twin experiments and suspended sediment concentrations (SSCs) retrieved from the Geostationary Ocean Color Imager (GOCI) in practical experiments. In the twin experiments, the sensitivity of the estimated ICs to several influential factors is discussed. The results demonstrate that the conjugate descent algorithm of Fletcher is proven to be better than the steepest descent, finite memory BFGS, and five other conjugate gradient algorithms in estimating the ICs; the estimated ICs are sensitive to initial guess values, and appropriate initial values are necessary for improving the efficiency of convergence and obtaining good results. Additionally, the errors of observations can significantly influence the estimated results. In contrast, the estimated results are not very sensitive to cloud coverage, errors in the background flow field, and length of the assimilation time window. In practical experiments, according to the conclusions of twin experiments, an improved 3D SSTM with the adjoint method is developed for Hangzhou Bay, and the surface GOCI-retrieved SSCs during typical neap and spring tidal cycles are assimilated to estimate the practical ICs. The experimental results imply that with the present estimation method, more accurate ICs can be obtained, which indicates that the adjoint method is effective in the estimation of the ICs in SSTMs. Furthermore, this study verifies that accurate ICs are critical for the numerical modeling of SSCs on the tidal cycle scale. This study is not only useful for further improving the accuracy of ICs in SSTMs but also suggestive for the initialization schemes of other matter transport models.
... However, in many cases, the observed tides are modulated by some non-tidal processes, such as the changes in bed friction, surface slope, vegetation may alter tidal properties (Horsburgh and Wilson, 2007;Jay, 2009;Jay et al., 2010). This phenomenon has also been noted by some scholars, and related research has been conducted to improve the classical harmonic analysis (Jin et al., 2015;Liu et al., 2010;Ramp et al., 2010;Zhao et al., 2010;Xu et al., 2011;Zhang et al., 2011;Guo et al., 2012;Huan et al., 2012;Xu et al., 2013;Gao et al., 2015;Gao et al., 2017;Xu et al., 2016). Jin et al. (2018) proposed EHA to optimize the classical harmonic analysis. ...
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The nodal cycle significantly affects the variation of sea level, which plays an important role in the design and plan of the coastal engineering, including coastal structures, harbor setting up and bay estuary engineering. Traditionally, the amplitude of the M2 nodal cycle is taken as constant in previous studies, but the amplitude of the M2 nodal cycle at San Francisco is nonstationary and temporally varying, because of the changes in physical properties of ocean and coastal morphology. Furthermore, the temporally varying amplitude of the M2 nodal cycle is difficult to be accurately extracted by using the conventional methods. In this study, a novel approach, namely enhanced harmonic analysis (EHA), is used to estimate the temporal variation in the amplitude of the M2 nodal cycle at San Francisco by analyzing the 116-year sea level observations. In the EHA, the independent point scheme and cubic spline interpolation are used. Considering the signal-to-noise ratios of the M2 nodal cycle and the long-term trend, the optimal number of the independent points in EHA is 10. The estimated results show that the 18.61-year nodal amplitude of the M2 tide have significantly temporal variations, with about 28-year and 42-year periods. In addition, the long-term trend of the M2 tidal amplitude is about 34.63 mm/century. Using the EHA with 10 independent points, the root-mean-square error between the observed and estimated monthly M2 tidal amplitude is 5.85 mm, which is decreased by 29.09% compared with that without considering the temporally varying amplitude of the M2 nodal cycle. The consideration of the temporal variations in the amplitudes of the M2 nodal cycle and the accurate extraction using EHA will have important significance for improving the precision of long-term sea level prediction and providing the helpful information for the design of the coastal engineering.
... Nevertheless, Zhang and Wang (2014) concluded that the efficiency of the L-BFGS was better than that of the GD for simple conditions in two-dimensional tidal models. Jin et al. (2015) stated that inversion results using the L-BFGS were closer to prescribed values than those using GD. However, Lu and Zhang (2006) and Zhang et al. (2011) found that GD was more efficient in the estimation of spatially varying bottom friction coefficient in a tidal model. ...
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Temporal vertical eddy viscosity coefficient (VEVC) in an Ekman layer model is estimated using an adjoint method. Twin experiments are carried out to investigate the influences of several factors on inversion results, and the conclusions of twin experiments are 1) the adjoint method is a capable method to estimate different kinds of temporal distributions of VEVCs; 2) the gradient descent algorithm is better than CONMIN and L-BFGS for the present problem, although the posterior two algorithms perform better on convergence efficiency; 3) inversion results are sensitive to initial guesses; 4) the model is applicable to different wind conditions; 5) the inversion result with thick boundary layer depth (BLD) is slightly better than thin BLD; 6) inversion results are more sensitive to observations in upper layers than those in lower layers; 7) inversion results are still acceptable when data noise exists, indicating the method can sustain noise to a certain degree; 8) a regularization method is proved to be useful to improve the results for present problem; and 9) the present method can tolerate the existence of balance errors due to the imperfection of governing equations. The methodology is further validated in practical experiments where Ekman currents are derived from Bermuda Testbed Mooring data and assimilated. Modeled Ekman currents coincide well with observed ones, especially for upper layers. The results demonstrate that the assumptions of depth dependence and time dependence are equally important for VEVCs. The feasibility of the typical Ekman model, the imperfection of Ekman balance equations, and the deficiencies of the present method are discussed. This method provides a potential way to realize the time variations of VEVCs in ocean models.
... As a result, it will lead to continuous harmonic results directly rather than manual interpolations. The philosophy of the independent point scheme (IPS) has been put forward in some studies to deal with the ill-posedness of the inverse problem, for 1D (Zhang and Lu 2010;Gao et al. 2013) and 2D parameters (Lu and Zhang 2006;Jin et al. 2015). Readers who are interested in this issue are referred to Pan et al. (2017) and Guo et al. (2017) for more details. ...
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... The important factors that affect the result of IPS are the selection of independent points and interpolation format. Studies, such as [24,25], have already coupled IPs distribution scheme with Cressman interpolation aiming at capturing more accurate results in the solutions and parameter inversions. Obviously, the optimal IPS distribution scheme matched with different interpolation should be not necessarily the same, due to the different interpolation effect. ...
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... Several studies have been done regarding the application of the L-BFGS method in adjoint models Jin et al., 2015). Because of the high complexity of cost functions in the control variable space and limitation of observations, sometimes the L-BFGS method fails to be a relatively better gradient related method than the steepest decent method . ...
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... on the BFGS algorithm described by Liu and Nocedal [51] coupled with a quadratic interpolation line search [52]. Generally speaking, this latter has proved to be particularly effective in these recent years in the area of inversion (see535455 to name but a few) due to its effectiveness in minimizing nonlinear problems [56]. The two-dimensional domain is a square of 2 cm length. ...
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SUMMARYA three-dimensional internal tidal model involving the adjoint method is constructed based on the nonlinear, time-dependent, free-surface hydrodynamic equations in spherical coordinates horizontally, and isopycnic coordinates vertically, subject to the hydrostatic approximations. This model consists of two submodels: the forward model is used for the simulation of internal tides, while the adjoint model is used for optimization of modal parameters. Mode splitting technique is employed in both forward and adjoint models. In this model, the adjoint method is employed to estimate model parameters by assimilating the interior observations. As a preliminary feasibility study, a set of ideal experiments with the model-generated pseudo-observations of surface currents are performed to invert the open boundary conditions (OBCs). In the ideal experiments, 14 kinds of bottom topographies and six kinds of predetermined distributions of OBCs are considered to examine their influence on experiment results. The inversion obtained satisfying results and all the predetermined distributions were successfully inverted. Analysis of results suggests the following: in the case where the spatial variation of the OBC distribution is great or the open boundary is close to a rough topography, the results will be comparatively poor, but still satisfactory; both the tidal elevations and currents can be simulated very accurately with the surface currents at several observation points; the assimilation precision could be reliable and able to reflect both of the inversion and simulation results in the whole field. The performance and results of ideal experiments give a preliminary indication that the construction of this model is successful. Copyright © 2011 John Wiley & Sons, Ltd.
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Based on the theory of inverse problem, the optimization of open boundary conditions (OBCs) in a 3D internal tidal model is investigated with the adjoint method. Fourier coefficients of internal tide on four open boundaries, which are regarded as OBCs, are inverted simultaneously. During the optimization, the steepest descent method is used to minimize cost function. The reasonability and feasibility of the model are tested by twin experiments (TEs). In TE1, OBCs on four open boundaries are successfully inverted by using independent point (IP) strategy, suggesting that IP strategy is useful in parameter estimation. Results of TE2 indicate that the model is effective even by assimilating inaccurate “observations.” Based on conclusions of TEs, the internal tide around Hawaii is simulated by assimilating T/P data in practical experiment. The simulated cochart shows good agreement with that obtained from the Oregon State University tidal model and T/P observations. Careful inspection shows that the major difference between simulated results and OSU model results is short-scale fluctuations superposed on coamplitude lines, which can be treated as the surface manifestation modulated by the internal tide. The computed surface manifestation along T/P tracks is comparable to the estimation in previous work.
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Differential equations, boundary, and discontinuity conditions are obtained which relate the internal tide to the surface tide in a two-layer system. Solutions of these equations give internal tides which may be large compared to the surface tide. In the coastal region these internal tides are standing waves and further offshore they attain the characteristics of progressive waves traveling seaward. DOI: 10.1111/j.2153-3490.1960.tb01283.x
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The system of objective weather map analysis used at the Joint Numerical Weather Prediction Unit is described. It is an integral part of the automatic data processing system, and is designed to operate with a minimum of manual supervision. The analysis method, based mainly on the method of Bergthorssen and Dooos, is essentially a method of applying corrections to a first guess field. The corrections are determined from a comparison of the data with the interpolated value of the guess field at the observation point. For the analysis of the heights of a pressure surface the reported wind is taken into account in determining the lateral gradient of the correction to be applied. A series of scans of the field is made, each scan consisting of application of corrections on a smaller lateral scale than during the previous scan. The analysis system is very flexible, and has been used to analyze many different types of variables. An example of horizontal divergence computed from a direct wind analysis is ...
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The adjoint method is used to assimilate observations into a quasi-geostrophic ocean model for a midlatitude jet. The domain has four open boundaries. Control variables used in this study are the lateral boundary values of stream function and relative vorticity. As a basic step, simulated data are assimilated (“identical-twin” approach), and the effects of reducing the amount of observations as well as changing their distribution in space and time are investigated. Special attention is paid to the problem of how well the unobserved parts of the model trajectory are resolved. First, data are assimilated as two-dimensional maps at certain time intervals. Subsequently, continuous assimilation is performed along satellite ground tracks. The solution deteriorates somewhat in the satellite scenario, for which the data set is relatively sparse. However, the model can still be well fitted to the “truth.” It is also shown that the deeper layers are constrained by the upper layer information.
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The East China Sea and adjacent seas are one of the most significant generation regions of the M2 internal tide in the world's oceans. In the present study, we investigate the distribution and energetics of the M2 internal tide around the continental shelf edge in the East China Sea using a three-dimensional numerical model. The numerical experiment shows that M2 internal tides are effectively generated over prominent topographic features such as the subsurface ridges in the Bashi/Luzon and Tokara Straits, the ridges along the Ryukyu Island chain, and the continental shelf slope in the East China Sea, the former particularly so. All of these topographic features are characterized by steep slopes at the depth of the thermocline onto which the M2 barotropic tide is almost normally incident. The M2 internal tides propagating away from these multiple source regions interfere with each other to create a complicated wave pattern. It is found that the calculated pattern of the M2 internal tide agrees well with TOPEX/Poseidon altimeter observations. The conversion rate from M2 barotropic to baroclinic energy over the whole analyzed model domain is estimated to be 35 GW. Roughly 10% of the energy in the M2 surface tide incident on the prominent topographic features is converted to the M2 internal tide, although about half of the M2 internal tidal energy is subject to local dissipation in close proximity to the generation sites.