Next Article in Journal
A Higher-Order Numerical Scheme for Two-Dimensional Nonlinear Fractional Volterra Integral Equations with Uniform Accuracy
Previous Article in Journal
Even-Order Neutral Delay Differential Equations with Noncanonical Operator: New Oscillation Criteria
 
 
Font Type:
Arial Georgia Verdana
Font Size:
Aa Aa Aa
Line Spacing:
Column Width:
Background:
Article

Regularization for a Sideways Problem of the Non-Homogeneous Fractional Diffusion Equation

1
School of Science, China University of Petroleum (East China), Qingdao 266580, China
2
Department of Mathematics, Northwest Normal University, Lanzhou 730070, China
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Fractal Fract. 2022, 6(6), 312; https://doi.org/10.3390/fractalfract6060312
Submission received: 11 May 2022 / Revised: 30 May 2022 / Accepted: 31 May 2022 / Published: 2 June 2022
(This article belongs to the Topic Fractional Calculus: Theory and Applications)

Abstract

:
In this article, we investigate a sideways problem of the non-homogeneous time-fractional diffusion equation, which is highly ill-posed. Such a model is obtained from the classical non-homogeneous sideways heat equation by replacing the first-order time derivative by the Caputo fractional derivative. We achieve the result of conditional stability under an a priori assumption. Two regularization strategies, based on the truncation of high frequency components, are constructed for solving the inverse problem in the presence of noisy data, and the corresponding error estimates are proved.

1. Introduction

Fractional partial differential equations arose from the studies of Lévy motion [1], continuous random walk [2] and high-frequency financial data [3], which has a wide range of applications in some scientific fields, such as chemistry, physics, mechanical engineering, fluid mechanics, signal processing and systems identification, control theory, electron transportation, viscoelasticity, image processing, and so on [4,5,6,7,8,9,10,11,12,13]. Moreover, fractional derivatives have been found to be more flexible in describing some practical phenomena than the traditional integer-order derivatives. In particular, fractional diffusion equations play an extremely important role in the study of some anomalous diffusion processes. These equations can describe the dynamics of various non-local and complex systems. Kinds of anomalous diffusion can be modeled by the following time-fractional diffusion equation: find the temperature u ( x , t ) from known boundary temperature u ( 1 , t ) = ψ ( t ) measurements satisfying the following system
ν u t ν u x x = 0 , x > 0 , t > 0 , u ( x , 0 ) = 0 , x > 0 , u ( 1 , t ) = ψ ( t ) , t > 0 , u ( x , t ) x b o u n d e d ,
where ψ ( t ) is given function (usually in L 2 ( R ) ) , ν u t ν is the Caputo fractional derivative of order ν ( 0 < ν 1 ) defined by [14]
ν u t ν = 1 Γ ( 1 ν ) 0 t u ( x , s ) s d s ( t s ) ν , 0 < ν < 1 ,
ν u t ν = u ( x , t ) t , ν = 1 .
The problem (1) in the case of ν = 1 , i.e., the following problem
u t u x x = 0 , x > 0 , t > 0 , u ( x , 0 ) = 0 , x > 0 , u ( 1 , t ) = φ ( t ) , t > 0 , u ( x , t ) x b o u n d e d ,
has been studied extensively in recent decades by many methods [15,16,17,18,19,20,21,22,23,24,25,26,27,28]. Tuan et al. [29] and Triet et al. [30] extended this work to the non-linear case.
When 0 < ν < 1 , Xiong et al. [31,32] proposed an optimal filtering regularization method for calculating an approximate solution of the fractional sideways heat equation where the spatial domain is the interval [0, 1]. Li et al. [33] tackled the inverse problem of recovering the temperature and flux distribution in the domain 0 x < 1 for (1) from the boundary data at x = 1 , but the conditional stability result is not given. Zheng et al. [34,35,36] obtains a stable estimate of temperature distribution by utilizing the spectral regularization method, and numerical example shows that the computational effect of their methods are satisfactory. Zhang [37] applied a Tikhonov-type regularized method to construct an approximate solution and overcome the ill-posedness of (1). The a-posteriori convergence estimates of logarithmic and double logarithmic types for the regularized method are derived. Moreover, the authors verify the effectiveness of their method by doing the numerical experiments. Furthermore, there are also some articles that discuss the fractional sideways heat equation in 2-dimensional and higher-dimensions in space (see, e.g., [38,39,40,41,42,43] and the references therein).
To the best of our knowledge, few investigations has been performed with respect to a sideways problem of the non-homogeneous diffusion equation, and estimating the heat flux at the inaccessible surface is more difficult than estimating temperature. Liu and Chang in [44] addressed a three-dimensional non-homogeneous sideways heat equation in a cuboid by a Fourier sine series method, and the analysis of the regularization parameter and the stability of solution was worked out. According to them, this method is quite accurate. Luan in [45] discussed the two-dimensional non-homogeneous heat equation in the presence of a general source term, and proposed a kernel regularization method to recover the temperature and heat flux distribution from the given data. However, the above two articles only consider the case of integer order. Hence, in contrast to the previous work, we consider a sideways problem of the non-homogeneous time-fractional diffusion equation, which occurs in many applications related to reaction-diffusion
α u t α u x x = f ( x , t ) , x > 0 , t > 0 , u ( x , 0 ) = 0 , x > 0 , u ( 1 , t ) = g ( t ) , t > 0 , u ( x , t ) x b o u n d e d ,
where the function f ( x , t ) is the heat source density. We first obtain an analytical solution to (5) via Fourier transform, and give the result of conditional stability under an a priori assumption. Due to the problem considered is severely ill-posed, it is impossible to solve it using classical numerical methods. Therefore, we propose dynamic spectral and Fourier regularization method, the goal here consists of recovering not only the temperature but also the heat flux distribution from the given data. Furthermore, for both regularization strategies, in the presence of noisy data, we establish and prove the stability and convergence estimates in the whole domain, i.e., including the case 0 < x < 1 and the case x = 1 .
The remainder of the paper is organized as follows: in Section 2, we give an analysis on the ill-posedness of the non-homogeneous fractional sideways heat equation. The conditional stability result is then given in Section 3. In Section 4 and Section 5, error estimates for determination of temperature and flux distribute are derived. Finally, we draw a conclusion to our method.

2. Mathematical Analysis of the Problem

In order to simplify the discussion, our theoretical analysis will be performed in L 2 ( R ) and define all functions to be zero for t < 0 . Let g ^ denote the Fourier transform of g ( t ) defined by
g ^ ( ξ ) = : 1 2 π g ( t ) e i ξ t d t ,
and · p denotes the norm in Sobolev space H p ( R ) defined by
u ( 0 , · ) p : = ( 1 + ξ 2 ) p | u ^ ( 0 , ξ ) | 2 d ξ 1 2 .
When p = 0 , · p = · denotes the L 2 ( R ) norm. Furthermore, we introduce the following norm
f ( x , · ) L 2 ( 0 , 1 ; H p ( R ) ) = 0 1 f ( x , · ) p 2 d x 1 2 .
Applying the Fourier transform with respect to t to both sides of (1), we obtain in the frequency space the following second order ordinary differential equation
u ^ x x ( x , ξ ) ( i ξ ) α u ^ ( x , ξ ) = f ^ ( x , ξ ) , ξ R , u ^ ( 1 , ξ ) = g ^ ( ξ ) , ξ R , u ^ ( x , ξ ) x b o u n d e d , ξ R .
The standard calculation procedure yields the solution of (6) as
u ^ ( x , ξ ) = e τ ( ξ ) ( 1 x ) g ^ ( ξ ) + x 1 f ^ ( s , ξ ) sinh τ ( ξ ) ( s x ) τ ( ξ ) d s , 0 x < 1 ,
and equivalently
u ( x , t ) = 1 2 π e τ ( ξ ) ( 1 x ) g ^ ( ξ ) + x 1 f ^ ( s , ξ ) sinh τ ( ξ ) ( s x ) τ ( ξ ) d s e i ξ t d ξ , 0 x < 1 ,
where
τ ( ξ ) : = ( i ξ ) α 2 = | ξ | α 2 cos ( α π 4 ) + i s i g n ( ξ ) sin ( α π 4 ) , ξ R .
Note that the real part of τ ( ξ ) is increasing positive function of ξ . Hence, the term | e ( 1 x ) τ ( ξ ) | and | sinh τ ( ξ ) ( s x ) | increase rather quickly when | ξ | , small errors in the data can blow up and ultimately destroy the solution for x [ 0 , 1 ) . Comparing this with homogeneous fractional sideways heat equation [31], it is no doubt that the problem (5) is much more ill-posed, and some regularization methods are in order.
Remark 1.
We do not consider the case f ( x , t ) = 0 in this paper. In fact, if f ( x , t ) = 0 , our problem is a homogeneous time-fractional sideways heat problem. We only note that, using our method, we obtain again the results of [33].
Remark 2.
By using the Fourier transform, the solution of general problem (5) where the data g is fixed at an specific point x 0 ( 0 , 1 ] , can be expressed as
u ^ ( x , ξ ) = e τ ( ξ ) ( x 0 x ) g ^ ( ξ ) + x x 0 f ^ ( s , ξ ) sinh τ ( ξ ) ( s x ) τ ( ξ ) d s , 0 x < 1 .
If we put x 0 = 1 in (10), we will obtain (7). In this context, the similar property can be acquired for this general problem and it is also an ill-posed problem. Furthermore, the similarity in (10) and (7) indicates that the methods using in the present paper are also applicable to solve the general problem.
Lemma 1
([45]). For arbitrary z C , x [ 0 , 1 ) and η ( x , 1 ] , we have
| sinh ( η x ) z z | e ( η x ) ( z ) | z | ,
| sinh ( η x ) z z | ( η x ) e ( η x ) | z | ,
| cosh ( x z ) | e x ( z ) e x | z | ,
where ( z ) denotes the real parts of z.
Lemma 2
([45]). For arbitrary c , d , p > 0 , the following inequality holds
( c + d ) p c p + d p , 0 < p 1 , 2 p 1 ( c p + d p ) , p > 1 .
Lemma 3.
If s 0 , then the function h ( s ) = e ( 1 x ) s s gets its minimum h min = ( 1 x ) e at s = 1 1 x .
So as to acquire a more sharp convergence, we use the following a priori condition
u ( 0 , · ) E .
Furthermore, since the sinh ( · ) function is exponentially increasing, we must find a sharply decreasing function to suppress its growth. Therefore, we also give the following assumption
0 1 | f ^ ( s , ξ ) | 2 d s < e 3 | ξ | α 2 , ξ R .
and the measured data ( g δ , f δ ) satisfy
g g δ + f f δ L 2 ( 0 , 1 ; L 2 ( R ) ) δ .
Throughout this paper, we denote the real part and imaginary part of τ ( ξ ) as follows
a : = ( τ ( ξ ) ) , b : = ( τ ( ξ ) ) .

3. A Conditional Stability Estimate

The object of stability estimates is to describe how much the development of solution from data magnifies errors, when noise contaminated the data. Next, we give the main results of this part.
Theorem 1.
Suppose that u ^ ( x , ξ ) given by (7) be the exact solution of problem (5) in the frequency space, and (16) is satisfied, then the following estimate holds for 0 x < 1
u ( x , t ) C 1 ( g ^ 2 + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 ) + 2 x + 2 u ^ ( 0 , ξ ) 2 2 x ( g ^ 2 x + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 x ) + C 2 f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 .
where C 1 and C 2 are constants that only depends on x.
Proof. 
By the Parseval’s identity, we have
u ( x , t ) 2 = u ^ ( x , ξ ) 2 = | ξ | 1 | e τ ( 1 x ) g ^ + x 1 f ^ sinh τ ( s x ) τ d s | 2 d ξ A 1 + | ξ | > 1 | e τ ( 1 x ) g ^ + x 1 f ^ sinh τ ( s x ) τ d s | 2 A 2 d ξ .
Next, we divide the argument into two steps.
Step 1. Estimate the term A 1 in (18). By Lemma 2, we have
A 1 2 | ξ | 1 | e τ ( 1 x ) g ^ | 2 d ξ A 11 + 2 | ξ | 1 | x 1 f ^ sinh τ ( s x ) τ d s | 2 d ξ A 12 .
Note that
| τ | = | ξ | α 2 1 ,
we obtain
A 11 2 | ξ | 1 e 2 | τ | ( 1 x ) | g ^ | 2 d ξ 2 e 2 ( 1 x ) g ^ 2 .
Using Cauchy–Schwarz integral inequality, (12) yields
A 12 2 | ξ | 1 x 1 | f ^ | 2 d s x 1 | sinh ( τ ( s x ) ) τ | 2 d s d ξ 2 | ξ | 1 x 1 | f ^ | 2 d s x 1 e 2 | τ | ( s x ) d s d ξ e 2 ( 1 x ) f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 .
Substituting (21) and (22) into (19), we obtain
A 1 C 1 ( g ^ 2 + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 ) ,
where
C 1 = 2 e 2 ( 1 x ) .
Step 2. Estimate the term A 2 in (18). Again, in view of Lemma 2, we have
A 2 2 | ξ | > 1 | e τ ( 1 x ) g ^ | 2 d ξ A 21 + 2 | ξ | > 1 | x 1 f ^ sinh τ ( s x ) τ d s | 2 d ξ A 22 .
We first estimate A 21 . Using (7) and Lemma 2, we have
A 21 = 2 | ξ | > 1 | e τ x u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ | 2 d ξ 4 | ξ | > 1 | e τ x | 2 | u ^ ( 0 , ξ ) | 2 d ξ A 21 ˜ + 4 | ξ | > 1 | e τ x | 2 | 0 1 f ^ sinh ( τ s ) τ d s | 2 d ξ A 22 ˜ .
By (17), Lemma 2, Hölder inequality, we have
A 21 ˜ = | ξ | > 1 | u ^ ( 0 , ξ ) | 2 1 x e 2 a | u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s + 0 1 f ^ sinh ( τ s ) τ d s | 2 x d ξ | ξ | > 1 ( | u ^ ( 0 , ξ ) | 2 ) 1 x [ 2 e 2 a | u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s | 2 x + 2 e 2 a | 0 1 f ^ sinh ( τ s ) τ d s | 2 x ] d ξ = | ξ | > 1 ( | u ^ ( 0 , ξ ) | 2 ) 1 x 2 e 2 a | u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s | 2 x d ξ + | ξ | > 1 ( | u ^ ( 0 , ξ ) | 2 ) 1 x 2 e 2 a | 0 1 f ^ sinh ( τ s ) τ d s | 2 x d ξ | ξ | > 1 | u ^ ( 0 , ξ ) | 2 d ξ 1 x | ξ | > 1 2 e 2 a | u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s | 2 d ξ x + | ξ | > 1 | u ^ ( 0 , ξ ) | 2 d ξ 1 x | ξ | > 1 2 e 2 a | 0 1 f ^ sinh ( τ s ) τ d s | 2 d ξ x .
By. Cauchy–Schwarz integral inequality and (11), we obtain
2 e 2 a | 0 1 f ^ sinh ( τ s ) τ d s | 2 2 e 2 a 0 1 | f ^ | 2 d s 0 1 | sinh ( τ s ) τ | 2 d s 2 e 2 a 0 1 | f ^ | 2 d s 0 1 e 2 s a | τ | 2 d s 2 0 1 | f ^ | 2 d s 1 2 a | τ | 2 .
Therefore,
A 21 ˜ | ξ | > 1 | u ^ ( 0 , ξ ) | 2 d ξ 1 x | ξ | > 1 | 2 g ^ | 2 d ξ x + | ξ | > 1 | u ^ ( 0 , ξ ) | 2 d ξ 1 x | ξ | > 1 2 0 1 | f ^ | 2 d s 1 2 a | τ | 2 d ξ x u ^ ( 0 , ξ ) 2 2 x 2 g ^ 2 x + 2 x u ^ ( 0 , ξ ) 2 2 x f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 x = 2 x u ^ ( 0 , ξ ) 2 2 x ( g ^ 2 x + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 x ) .
Likewise, we have
A 22 ˜ | ξ | > 1 | 0 1 f ^ sinh ( τ s ) τ d s | 2 d ξ 1 x | ξ | > 1 e 2 a | 0 1 f ^ sinh ( τ s ) τ d s | 2 d ξ x | ξ | > 1 0 1 | f ^ | 2 d s 0 1 e 2 | τ | s d s 1 x | ξ | > 1 ( 0 1 | f ^ | 2 d s ) 1 2 a | τ | 2 d ξ x | ξ | > 1 0 1 | f ^ | 2 d s e 2 | τ | 2 | τ | 1 x f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 x e 1 x f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 .
Combining the estimates of A 21 ˜ with A 22 ˜ , we obtain
A 21 2 x + 2 u ^ ( 0 , ξ ) 2 2 x ( g ^ 2 x + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 x ) + 4 e 1 x f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 .
Next, we estimate A 22 . By Cauchy–Schwarz integral inequality, (12) and Lemma 3, we obtain
A 22 2 | ξ | > 1 x 1 | f ^ | 2 d s x 1 | sinh ( τ ( s x ) ) τ | 2 d s d ξ 2 | ξ | > 1 x 1 | f ^ | 2 d s x 1 e 2 | τ | ( s x ) d s d ξ 2 | ξ | > 1 x 1 | f ^ | 2 d s e 2 | τ | ( 1 x ) 2 | τ | d ξ 2 ( 1 x ) e f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 .
Inserting (27) and (28) into (25), we have
A 2 2 x + 2 u ^ ( 0 , ξ ) 2 2 x ( g ^ 2 x + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 x ) + C 2 f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 ,
where
C 2 = 4 e 1 x + 2 ( 1 x ) e .
Substituting (23) and (29) into (18), and using Lemma 2, we obtain
u ^ ( x , ξ ) A 1 + A 2 C 1 ( g ^ 2 + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 ) + 2 x + 2 u ^ ( 0 , ξ ) 2 2 x ( g ^ 2 x + f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 x ) + C 2 f ^ L 2 ( 0 , 1 ; L 2 ( R ) ) 2 ,
where C 1 and C 2 is given by (24) and (30), respectively. □

4. Determination of the Temperature Distribution

In this part, we use the dynamic spectral method to recover the temperature distribution from the measured data. Since the matter of instability lies in the noise of data in the high frequency components, naturally a “corrector” is added to these in order to control their growth. As a result, one may obtain a stable approximation. Suppose β is the regularization parameter, motivated by [31], we contemplate the following regularized solutions in the frequency domain:
  • Method 1
u ^ β δ ( x , ξ ) = e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s , e a ( 1 x ) β , e 2 a ( 1 x ) β [ e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s ] , e a ( 1 x ) < β .
  • Method 2
v ^ β δ ( x , ξ ) = e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s , e a ( 1 x ) β , e a ( 1 x ) β [ e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s ] , e a ( 1 x ) < β .
  • Method 3
w ^ β δ ( x , ξ ) = e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s , e a ( 1 x ) β , e a 2 ( 1 x ) β 1 4 [ e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s ] , e a ( 1 x ) < β .
Generally,
μ ^ β δ ( x , ξ ) = e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s , e a ( 1 x ) β , e γ a ( 1 x ) β γ [ e τ ( ξ ) ( 1 x ) g ^ δ ( ξ ) + x 1 f ^ δ ( s , ξ ) sinh ( τ ( ξ ) ( s x ) ) τ ( ξ ) d s ] , e a ( 1 x ) < β ,
where γ > 0 is a real number. Because the three spectral methods are very similar, then we only give the properties of the first two methods.
Remark 3.
It is apparently that the regularization solutions approach the exact solution if β 0 as δ 0 .
Lemma 4.
If condition (14) and (15) hold, B ( ξ ) = u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s , then
B ( ξ ) E + N 1 ,
where N 1 is a constant.
Proof. 
Successively using the triangle inequality, (14), Cauchy–Schwarz integral inequality, (12) and (15), we obtain
B ( ξ ) u ^ ( 0 , ξ ) + 0 1 f ^ sinh ( τ s ) τ d s E + 0 1 | sinh ( τ s ) τ | 2 d s 0 1 | f ^ | 2 d s d ξ 1 2 E + 0 1 | s e s | τ | | 2 d s 0 1 | f ^ | 2 d s d ξ 1 2 E + 1 2 | ξ | α 2 e | ξ | α 2 d ξ 1 2 .
It is easy to know that the generalized integral on the right-hand side of the last inequality converges, here we introduce the notation
N 1 : = 1 2 | ξ | α 2 e | ξ | α 2 d ξ 1 2 .
Therefore,
B ( ξ ) E + N 1 ,
where N 1 is a constant. □
Theorem 2.
Let u ^ ( x , ξ ) given by (7) be the exact solution of problem (5) in the frequency space, u ^ β δ ( x , ξ ) given by (31) be the regularized solution, condition (14)–(16) hold. If the regularization parameter β is selected dynamically
β ( x ) = 2 2 x 2 x 2 x x 2 δ E + 2 N 1 2 ( 1 x ) .
Then, for a fixed x ( 0 , 1 ) , we have
u β δ ( x , · ) u ( x , · ) 2 1 x 2 x x 2 x x 2 δ x E + 2 N 1 1 x + δ ( 1 x ) e .
Proof. 
By the triangle inequality, we have
u β δ ( x , · ) u ( x , · ) u β δ ( x , · ) u β ( x , · ) I 1 + u β ( x , · ) u ( x , · ) I 2 .
Next, we divide the argument into two steps.
Step 1. Estimate the term I 1 in (38). It follows immediately from Parseval’s equality and the triangle inequality that
I 1 = u ^ β δ ( x , · ) u ^ β ( x , · ) = min 1 , e 2 a ( 1 x ) β [ e τ ( 1 x ) ( g ^ δ g ^ ) + x 1 ( f ^ δ f ^ ) sinh τ ( s x ) τ d s ] min 1 , e 2 a ( 1 x ) β e τ ( 1 x ) ( g ^ δ g ^ ) I 1 ¯ + min 1 , e 2 a ( 1 x ) β x 1 ( f ^ δ f ^ ) sinh τ ( s x ) τ d s I 2 ¯ .
By (17) and (16), we obtain
I 1 ¯ e 2 a ( 1 x ) β e ( a + b i ) ( 1 x ) ( g ^ δ g ^ ) e a ( 1 x ) < β = e ( a + b i ) ( 1 x ) β ( g ^ δ g ^ ) δ β 1 2 .
Using Cauchy–Schwarz integral inequality, (12), Lemma 3 and (16) yields
I 2 ¯ x 1 ( f ^ δ f ^ ) sinh τ ( x s ) τ d s x 1 | f ^ δ f ^ | 2 d s x 1 e 2 ( s x ) | τ | d s x 1 | f ^ δ f ^ | 2 d s e 2 ( 1 x ) | τ | 2 | τ | δ ( 1 x ) e .
Hence,
I 1 δ β 1 2 + δ ( 1 x ) e .
Step 2. Estimate the term I 2 in (38). Again, by the Parseval’s identity and the triangle inequality,
I 2 = u ^ β ( x , · ) u ^ ( x , · ) = min 1 , e 2 a ( 1 x ) β · e τ ( 1 x ) g ^ + x 1 f ^ sinh τ ( s x ) τ d s e τ ( 1 x ) g ^ + x 1 f ^ sinh τ ( s x ) τ d s 1 min 1 , e 2 a ( 1 x ) β e τ ( 1 x ) g ^ I 1 ˜ + 1 min { 1 , e 2 a ( 1 x ) β ) x 1 f ^ sinh τ ( s x ) τ d s I 2 ˜ .
We start by estimating the first term above. Let
B 1 ( a ) = 1 e 2 a ( 1 x ) β e a x .
Using (7) and (17), we obtain
I 1 ˜ = 1 min 1 , e 2 a ( 1 x ) β e τ x u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s sup e 2 a ( 1 x ) β B 1 ( a ) u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s .
By elementary calculations, it is easy to find the zero point a * of B 1 ( a ) satisfies
e 2 a * ( 1 x ) = β x 2 x ,
and a * maximize the function B 1 ( a ) . Thus,
B 1 ( a ) B 1 ( a * ) = 1 x 2 x β x 2 x x 2 ( 1 x ) .
Using Lemma 4, we have
I 1 ˜ 1 x 2 x β x 2 x x 2 ( 1 x ) E + N 1 .
Now we estimate I 2 ˜ . Using Cauchy–Schwarz integral inequality, (12), (17), (15), (40), (9) and (10) yields
I 2 ˜ 1 e 2 a ( 1 x ) β e a x x 1 f ^ sinh ( τ ( s x ) ) τ d s e a x sup e 2 a ( 1 x ) β B 1 ( a ) x 1 | f ^ | 2 d s x 1 e 2 | τ | ( s x ) d s e 2 a x d ξ 1 2 sup e 2 a ( 1 x ) β B 1 ( a ) x 1 | f ^ | 2 d s e 2 | τ | ( 1 x ) 2 | τ | e 2 | τ | x d ξ 1 2 1 x 2 x β x 2 x x 2 ( 1 x ) N 1 .
Therefore,
I 2 1 x 2 x β x 2 x x 2 ( 1 x ) E + 2 N 1 .
Substituting (39) and (40) into (38), we obtain
u β δ ( x , · ) u ( x , · )
δ β 1 2 + δ ( 1 x ) e + 1 x 2 x β x 2 x x 2 ( 1 x ) E + 2 N 1 : = h 1 ( β ) .
Minimizing the right-hand side of (42) with respect to β , we can obtain (36). Hence, (37) hold. □
Theorem 3.
Let u ^ ( x , ξ ) given by (7) be the exact solution of problem (5) in the frequency space, v ^ β δ ( x , ξ ) given by (32) be the regularized solution, condition (14)–(16) hold. If the regularization parameter β is selected dynamically
β ( x ) = x 2 δ E + 2 N 1 2 ( 1 x ) .
Then, for a fixed x ( 0 , 1 ) , we have
v β δ ( x , · ) u ( x , · ) δ x E + 2 N 1 1 x + δ ( 1 x ) e .
Proof. 
By the triangle inequality, we have
v β δ ( x , · ) u ( x , · ) v β δ ( x , · ) v β ( x , · ) I 3 + v β ( x , · ) u ( x , · ) I 4 .
Next, we divide the argument into two steps.
Step 1. Estimate the term I 3 in (45). Taking a similar procedure of the estimate of I 1 , we have
I 3 = v ^ β δ ( x , · ) v ^ β ( x , · ) min 1 , e a ( 1 x ) β e τ ( 1 x ) ( g ^ δ g ^ ) + min 1 , e a ( 1 x ) β x 1 ( f ^ δ f ^ ) sinh τ ( s x ) τ d s e a ( 1 x ) β e ( a + b i ) ( 1 x ) ( g ^ δ g ^ ) e a ( 1 x ) < β + x 1 ( f ^ δ f ^ ) sinh τ ( s x ) τ d s δ β 1 2 + δ ( 1 x ) e .
Step 2. Estimate the term I 4 in (45). By the Parseval’s identity, we have
I 4 = v ^ β ( x , · ) u ^ ( x , · ) 1 min 1 , e a ( 1 x ) β e τ ( 1 x ) g ^ I 3 ˜ + 1 min 1 , e a ( 1 x ) β x 1 f ^ sinh τ ( s x ) τ d s I 4 ˜ .
We start by estimating the first term above. Let
B 2 ( a ) = 1 e a ( 1 x ) β e a x .
Using (7) and (17), we obtain
I 3 ˜ = 1 min 1 , e a ( 1 x ) β e τ x u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s sup e a ( 1 x ) β B 2 ( a ) u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s .
By elementary calculations, it is easy to find the zero point a * of B 2 ( a ) satisfies
e a * ( 1 x ) = β x ,
and a * maximize the function B 2 ( a ) . Thus,
B 2 ( a ) B 2 ( a * ) = ( 1 x ) β x x 1 x .
By Lemma 4, we have
I 3 ˜ ( 1 x ) β x x 1 x E + N 1 .
Now we estimate I 4 ˜ . Using Cauchy–Schwarz integral inequality, (12), (17), (15), (9), (47) and (35) yields
I 4 ˜ 1 e a ( 1 x ) β e a x x 1 f ^ sinh τ ( x s ) τ d s e a x sup e a ( 1 x ) β B 2 ( a ) x 1 | f ^ | 2 d s x 1 e 2 | τ | ( s x ) d s e 2 a x d ξ 1 2 ( 1 x ) β x x 1 x N 1 .
Therefore,
I 4 ( 1 x ) β x x 1 x E + 2 N 1 .
Substituting (46) and (48) into (45), we obtain
v β δ ( x , · ) u ( x , · ) δ β 1 2 + δ ( 1 x ) e + ( 1 x ) β x x 1 x E + 2 N 1 : = h 2 ( β ) .
Minimizing the right-hand side of (49) with respect to β , we can obtain (43). Hence, (44) hold. □
Remark 4.
In Theorems 2 and 3, we choose the regularization parameter β to depend on the position of x, which will justify our use of the phrase “dynamic spectral”. Moreover, we can find that the estimate of Theorem 3 is better than the estimate of Theorem 2.
It is easy to see that two errors in Theorems 2 and 3 are not near to zero, if δ fixed and x tend to zero. Hence, the convergence of the approximate solution is very slow when x is in a neighborhood of zero. In addition, considering that the sinh ( · ) function is exponentially increasing, to retain the continuous dependence of the solution at x = 0 , we have to introduce some stronger a priori assumptions
u ( 0 , · ) p E , p > 0 ,
1 + ξ 2 p 0 1 | f ^ ( s , ξ ) | 2 d s < e 3 | ξ | α 2 , ξ R .
Next, we only give error estimate at x = 0 for (32).
Lemma 5.
Let condition (50) and (51) hold, B ˜ ( ξ ) = 1 + ξ 2 p 2 [ u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s ] , then
B ˜ ( ξ ) E + N 1 ,
where N 1 is a constant.
Theorem 4.
Let u ^ ( x , ξ ) given by (7) be the exact solution of problem (5) in the frequency space, v ^ β δ ( x , ξ ) given by (32) be the regularized solution, condition (16), (50), (51) hold. The regularization parameter β is chosen as
β = 1 C ( a * δ r ) 2 ,
where 0 < r < 1 , C ( a * ) = 2 p a * α + 2 p < 1 , a * is a constant. Then, the following inequality hold
v β δ ( 0 , · ) u ( 0 , · ) C ( a * ) δ 1 r + δ e + 1 C ( a * ) r ln 1 δ 2 p α E + 2 N 1 , p > 0 .
Proof. 
By the triangle inequality, we have
v β δ ( 0 , · ) u ( 0 , · ) v β δ ( 0 , · ) v β ( 0 , · ) I 5 + v β ( 0 , · ) u ( 0 , · ) I 6 .
Next, we divide the argument into two steps.
Step 1. Estimate the term I 5 in (54). In view of the Parseval’s equality, the triangle inequality, Cauchy–Schwarz integral inequality, (12), Lemma 3 and (16), we have
I 5 = v ^ β δ ( 0 , · ) v ^ β ( 0 , · ) min { 1 , e a β } e τ ( g ^ δ g ^ ) + min 1 , e a β 0 1 ( f ^ δ f ^ ) sinh ( τ s ) τ d s e a β e ( a + b i ) ( g ^ δ g ^ ) e a < β + 0 1 ( f ^ δ f ^ ) sinh ( τ s ) τ d s δ β 1 2 + 0 1 | f ^ δ f ^ | 2 d s 0 1 e 2 s | τ | d s d ξ 1 2 δ β 1 2 + δ e .
Step 2. Estimate the term I 6 in (54). By the Parseval’s equality and the triangle inequality, we obtain
I 6 = v ^ β ( 0 , · ) u ^ ( 0 , · ) 1 min 1 , e a β e τ g ^ I 5 ˜ + 1 min 1 , e a β 0 1 f ^ sinh ( τ s ) τ d s I 6 ˜ .
We start by estimating the first term above. Let
B 3 ( a ) = 1 e a β a 2 p α .
Using (7), and note that a | ξ | α 2 , we obtain
I 5 ˜ = 1 min 1 , e a β u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s sup e a β 1 e a β 1 + ξ 2 p 2 u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s 1 + ξ 2 p 2 sup e a β B 3 ( a ) u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s 1 + ξ 2 p 2 .
By elementary calculations, it is easy to find the zero point a * of B 3 ( a ) satisfies
e a * β = C ( a * ) ,
where
C ( a * ) = 2 p a * α + 2 p < 1 ,
and a * maximize the function B 3 ( a ) . Thus,
B 3 ( a ) B 3 ( a * ) = 1 C ( a * ) ln 1 β C ( a * ) 2 p α .
By Lemma 5, we obtain
I 5 ˜ [ 1 C ( a * ) ] ln 1 β C ( a * ) 2 p α E + N 1 .
Now we estimate I 6 ˜ . Using (56) and Lemma 5 yields
I 6 ˜ 1 e a β 1 + ξ 2 p 2 0 1 f ^ sinh ( τ s ) τ d s 1 + ξ 2 p 2 sup e a ( 1 x ) β B 3 ( a ) 0 1 f ^ sinh ( τ s ) τ d s 1 + ξ 2 p 2 1 C ( a * ) ln 1 β C ( a * ) 2 p α N 1 .
Therefore,
I 6 1 C ( a * ) ln 1 β C ( a * ) 2 p α E + 2 N 1 .
Then, by (54), we have
v β δ ( x , · ) u ( x , · ) δ β 1 2 + δ e + 1 C ( a * ) ln 1 β C ( a * ) 2 p α E + 2 N 1 = C ( a * ) δ 1 r + δ e + 1 C ( a * ) r ln 1 δ 2 p α E + 2 N 1 .
where C ( a * ) is given by (55). □
Remark 5.
If we replace the assumption (14) and (15) by (50) and (51), then the convergence u β δ ( x , · ) u ( x , · ) p and v β δ ( x , · ) u ( x , · ) p is also hold.
Remark 6.
From a theoretical point of view, Theorem 4 has obtained the stability estimate for the endpoint x = 0 , since lim δ 0 v β δ ( 0 , · ) u ( 0 , · ) = 0 .
Remark 7.
In 1987, Eldén [19] proved that it is impossible to obtain the error asymptotically better than logarithmic rate at x = 0 . So our estimates is reasonable, although the logarithmic term ln 1 δ implies the convergence rate is very slow.

5. Determination of Flux Structure and Error Estimate

In this section, we use the Fourier regularization method to recover the flux distribution from the measure data. Differentiating the variable x on the right-hand side of (7), we obtain the following formula for the heat flux, denoted by
u ^ x ( x , ξ ) = τ ( ξ ) e ( 1 x ) τ ( ξ ) g ^ δ x 1 f ^ δ cosh τ ( ξ ) ( s x ) d s , 0 x < 1 .
The method we adopt is to eliminate all high frequencies from the solution, and instead consider (5) for | ξ | ξ max . Then, we obtain a regularized solution
u ^ x δ , ξ max ( x , ξ ) = τ ( ξ ) e ( 1 x ) τ ( ξ ) g ^ δ x 1 f ^ δ cosh τ ( ξ ) ( s x ) d s χ max .
where ξ max is the regularization parameter, χ max is the characteristic function of the interval [ ξ max , ξ max ] .
Theorem 5.
Let u ^ ( x , ξ ) given by (7) be the exact solution of problem (5) in the frequency space, u ^ x δ , ξ max ( x , ξ ) given by (58) be the regularized solution, condition (14)–(16) hold. If the regularization parameter ξ max is selected by
ξ max = ln E δ 2 α .
Then for a fixed x ( 0 , 1 ) , we have
u x δ , ξ max ( x , · ) u x ( x , · ) 2 ln E δ + ( ln E δ ) 1 2 E 1 x δ x + ϵ 1 2 E x δ x E + N 1 + ln E δ 1 2 N 2 ,
where ϵ 1 = max { 1 x , ln E δ } , N 1 and N 2 are some constants.
Proof. 
By the triangle inequality, we have
u x δ , ξ max ( x , · ) u x ( x , · ) u x δ , ξ max ( x , · ) u x ξ max ( x , · ) J 1 + u x ξ max ( x , · ) u x ( x , · ) J 2 .
Next, we divide the argument into two steps.
Step 1. Estimate the term J 1 in (60). It follows immediately from Parseval’s equality and Lemma 2 that
J 1 = u ^ x δ , ξ max ( x , · ) u ^ x ξ max ( x , · ) = | ξ | ξ max | τ e τ ( 1 x ) ( g ^ g ^ δ ) + x 1 ( f ^ f ^ δ ) cosh τ ( s x ) d s | 2 d ξ 1 2 | ξ | ξ max 2 | τ e τ ( 1 x ) ( g ^ g ^ δ ) | 2 d ξ 1 2 J 1 ¯ + | ξ | ξ max 2 | x 1 ( f ^ f ^ δ ) cosh τ ( s x ) d s | 2 d ξ 1 2 J 2 ¯ .
By (16) and (59), we obtain
J 1 ¯ 2 δ sup | ξ | ξ max | τ e τ ( 1 x ) | 2 δ | τ | e | τ | ( 1 x ) 2 δ ξ max α 2 e ξ max α 2 ( 1 x ) = 2 E 1 x δ x ln E δ .
Using Cauchy–Schwarz integral inequality, (13), (59) and (16) yields
J 2 ¯ | ξ | ξ max 2 x 1 e 2 | τ | ( s x ) d s x 1 | f ^ f ^ δ | 2 d s d ξ 1 2 ξ max α 4 e ( 1 x ) ξ max α 2 f ^ f ^ δ L 2 ( 0 , 1 ; L 2 ( R ) ) ln E δ 1 2 E 1 x δ x .
Thus, by (61) and (62)
J 1 2 ln E δ + ( ln E δ ) 1 2 E 1 x δ x .
Step 2. Estimate the term J 2 in (60). Again, using the Parseval’s identity and Lemma 2, we have
J 2 = u ^ x ξ max ( x , · ) u ^ x ( x , · ) = | ξ | > ξ max | τ e τ ( 1 x ) g ^ + x 1 f ^ cosh τ ( s x ) d s | 2 d ξ 1 2 | ξ | > ξ max 2 | τ e τ ( 1 x ) g ^ | 2 d ξ 1 2 J 1 ˜ + | ξ | > ξ max 2 | x 1 f ^ cosh τ ( s x ) d s | 2 d ξ 1 2 J 2 ˜ .
We first estimate J 1 ˜ . Let
B 4 | ξ | = 2 | ξ | α 2 e x | ξ | α 2 .
By (7), we have
J 1 ˜ = | ξ | > ξ max 2 | τ e τ x u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s | 2 d ξ 1 2 sup | ξ | > ξ max B 4 | ξ | u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s .
By elementary calculations, it is easy to find the unique zero point | ξ * | of B 4 ( | ξ | ) is
| ξ * | = 1 x 2 α ,
and | ξ * | maximize the function B 4 | ξ | . Thus,
sup | ξ | > ξ max B 4 | ξ | = 2 | ξ * | α 2 e x | ξ * | α 2 2 | ξ * | α 2 e x ξ max α 2 , ξ max < | ξ * | , 2 ξ max α 2 e x ξ max α 2 , ξ max | ξ * | .
By (59), we have
sup | ξ | > ξ max B 4 | ξ | 1 x , ln E δ 2 e x ln E δ : = ϵ 1 2 E x δ x ,
where
ϵ 1 = max 1 x , ln E δ .
Therefore, by Lemma 4, we obtain
J 1 ˜ ϵ 1 2 E x δ x E + N 1 .
Now we estimate J 2 ˜ . Using Cauchy–Schwarz integral inequality, (13) and (15) yields
J 2 ˜ | ξ | > ξ max 2 x 1 e 2 | τ | ( s x ) d s x 1 | f ^ | 2 d s d ξ 1 2 | ξ | > ξ max 1 | ξ | α 2 e 2 | ξ | α 2 ( 1 x ) x 1 | f ^ | 2 d s d ξ 1 2 ξ max α 4 | ξ | > ξ max e 2 | ξ | α 2 ( 1 x ) e 3 | ξ | α 2 d ξ 1 2 .
Since the generalized integral on the right side of the last inequality converges for 0 < x < 1 , we introduce the notation
N 2 = | ξ | > ξ max e | ξ | α 2 d ξ 1 2 .
Using (59), we have
J 2 ˜ ln E δ 1 2 N 2 .
Thus,
J 2 ϵ 1 2 E x δ x E + N 1 + ln E δ 1 2 N 2 .
where ϵ 1 is given by (64). By substituting (63) and (66) into (60), we arrive at the final conclusion. □
Remark 8.
If we replace assumptions (14) and (15) by (50) and (51), then the convergence u x δ , ξ max ( x , · ) u x ( x , · ) p also holds.
Similarly, the accuracy of the regularized solution becomes progressively lower as x 0 , and then we use the condition (50) and (51) to give convergence estimate at x = 0 .
Theorem 6.
Let u ^ ( x , ξ ) given by (7) be the exact solution of problem (5) in the frequency space, u ^ x δ , ξ max ( x , ξ ) given by (58) be the regularized solution, condition (16), (50) and (51) hold. If the regularization parameter ξ max is selected by
ξ max = ln ( E δ ( ln E δ ) 2 p α ) 2 α .
Then, for p > α 2 , we have
u x δ , ξ max ( 0 , · ) u x ( 0 , · ) ( 2 ϵ 2 1 + ϵ 2 1 2 ) E ln E δ 2 p α + 2 ϵ 2 2 p α 1 E + N 1 + ϵ 2 1 2 + 2 p α N 2 ,
where ϵ 2 = ln ( E δ ( ln E δ ) 2 p α ) 1 , N 1 and N 2 are some constants.
Proof. 
By the triangle inequality, we have
u x δ , ξ max ( 0 , · ) u x ( 0 , · ) u x δ , ξ max ( 0 , · ) u x ξ max ( 0 , · ) J 3 + u x ξ max ( 0 , · ) u x ( 0 , · ) J 4 .
Next, we divide the argument into two steps.
Step 1. Estimate the term J 3 in (69). Taking a similar procedure of the estimate of J 1 , and by (67), we obtain
J 3 = u ^ x δ , ξ max ( 0 , · ) u ^ x ξ max ( 0 , · ) | ξ | ξ max 2 | τ e τ ( g ^ g ^ δ ) | 2 d ξ 1 2 + | ξ | ξ max 2 | 0 1 f ^ f ^ δ cosh ( τ s ) d s | 2 d ξ 1 2 2 δ sup | ξ | ξ max | τ e τ | + | ξ | ξ max 2 0 1 e 2 | τ | s d s 0 1 | f ^ f ^ δ | 2 d s d ξ 1 2 2 δ ξ max α 2 e ξ max α 2 + ξ max α 4 e ξ max α 2 f ^ δ f ^ L 2 ( 0 , 1 ; H p ( R ) ) ( 2 ϵ 2 1 + ϵ 2 1 2 ) E ln E δ 2 p α ,
where
ϵ 2 = ln ( E δ ( ln E δ ) 2 p α ) 1 .
Step 2. Estimate the term J 4 in (69). By Lemma 2, we have
J 4 = u ^ x ξ max ( 0 , · ) u ^ x ( 0 , · ) | ξ | > ξ max 2 | τ e τ g ^ | 2 d ξ 1 2 J 3 ˜ + | ξ | > ξ max 2 | 0 1 f ^ cosh ( τ s ) d s | 2 d ξ 1 2 J 4 ˜ .
We first estimate J 3 ˜ . By (7), (9), (67)and Lemma 5, we have
J 3 ˜ = | ξ | > ξ max 2 | ( 1 + ξ 2 ) p 2 τ u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s 1 + ξ 2 p 2 | 2 d ξ 1 2 2 ξ max α 2 p ( 1 + ξ 2 ) p 2 u ^ ( 0 , ξ ) 0 1 f ^ sinh ( τ s ) τ d s 2 ϵ 2 2 p α 1 E + N 1 .
Now we estimate J 4 ˜ . Using Cauchy–Schwarz integral inequality, (13), (9), (51), (67) and (65) yields
J 4 ˜ | ξ | > ξ max 2 1 + ξ 2 p 0 1 e 2 | τ | s d s 0 1 | f ^ | 2 d s 1 + ξ 2 p d ξ 1 2 | ξ | > ξ max | ξ | 2 p 1 | ξ | α 2 e 2 | ξ | α 2 0 1 | f ^ | 2 d s 1 + ξ 2 p d ξ 1 2 ξ max ( α 4 + p ) | ξ | > ξ max e | ξ | α 2 d ξ 1 2 = ϵ 2 1 2 + 2 p α N 2 .
Then
J 4 2 ϵ 2 2 p α 1 E + N 1 + ϵ 2 1 2 + 2 p α N 2 ,
where ϵ 2 is given by (71). The Theorem now follows from equations (69)–(72). □
Remark 9.
Since the regularization parameter ξ max as δ 0 , we can easily find that, for p > α 2 , ϵ 2 0 ( δ 0 ). In addition, note that for p > α 2 there hold
ln E δ ( ln E δ ) 2 p α ln E δ 2 p α = ln E δ 1 2 p α 2 p α ln ( ln E δ ) ln E δ 2 p α 0 , δ 0 .
Therefore,
lim δ 0 u x δ , ξ max ( 0 , · ) u x ( 0 , · ) = 0 , p > α 2 .
Remark 10.
In 2007, Qian [46] proved that it is impossible to obtain the error asymptotically better than logarithmic rate at x = 0 . So our estimates is reasonable.

6. Conclusions

In this paper, we have considered the problem of finding a function u ( x , t ) satisfying (5). This is a sideways problem for non-homogeneous fractional heat equation, and the problem is ill-posed. To regularize the problem, we propose the dynamic spectral method and Fourier method, which are rather simple and convenient for dealing with some ill-posed problems. Error estimations between the approximate solution and the exact one, established from noise data g δ and f δ , are given. In fact, the paper extends the work in [33]. It is worth noting that the obtained estimates are sufficient to prove the results, but most of them are quite rough and can be improved.
As we all know, the most common regularization methods are the Tikhonov method, iterative method, quasi-reversibility method, truncation method, quasi-boundary value method and spectral method. The main difference between these methods is their convergence order. We can compare the convergence rate of errors by using different methods to discuss the problem. In addition, the dynamic spectral method and Fourier method can easily be extended to multi-dimensional case, which needs further study.

Author Contributions

Formal analysis, Y.C. and Y.Q.; Supervision, X.X. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Written informed consent has been obtained from the patients to publish this paper.

Data Availability Statement

Not applicable.

Conflicts of Interest

The authors declare no conflict of interest.

References

  1. Meerschaert, M.M.; Scheffer, H.P. Semistable Lévy motion. Fract. Calc. Appl. Anal. 2002, 5, 27–54. [Google Scholar]
  2. Barkai, E.; Metzler, R.; Klafter, J. From continuous time random walks to the fractional Fokker-Planck equation. Phys. Rev. E Stat. Phys. Plasmas Fluids Relat. Interdiscip. Top. 2000, 61, 132–138. [Google Scholar] [CrossRef] [PubMed]
  3. Raberto, M.; Scalas, E.; Mainardi, F. Waiting-times and returns in high-frequency financial data: An empirical study. Phys. A Stat. Mech. Its Appl. 2002, 314, 749–755. [Google Scholar] [CrossRef] [Green Version]
  4. Sabatier, J.; Lanusse, P.; Melchior, P.; Oustaloup, A. Fractional Order Differentiation and Robust Control Design; Springer: Dordrecht, The Netherlands, 2015. [Google Scholar]
  5. Das, S.; Pan, I. Fractional Order Signal Processing; Springer: Berlin/Heidelberg, Germany, 2012. [Google Scholar]
  6. Vilela Mendes, R. A fractional calculus interpretation of the fractional volatility model. Nonlinear Dyn. 2009, 55, 395–399. [Google Scholar] [CrossRef]
  7. Roul, P. Analytical approach for nonlinear partial differential equations of fractional order. Commun. Theor. Phys. 2013, 60, 269–277. [Google Scholar] [CrossRef]
  8. Roul, P. A high accuracy numerical method and its convergence for time-fractional Black-Scholes equation governing European options. Appl. Numer. Math. 2020, 151, 472–493. [Google Scholar] [CrossRef]
  9. Li, C.P.; Wang, Z. The discontinuous Galerkin finite element method for Caputo-type nonlinear conservation law. Math. Comput. Simul. 2020, 169, 51–73. [Google Scholar] [CrossRef]
  10. Sun, H.G.; Chen, Y.Q.; Chen, W. Random-order fractional differential equation models. Signal Process. 2011, 91, 525–530. [Google Scholar] [CrossRef]
  11. Atangana, A.; Qureshi, S. Modeling attractors of chaotic dynamical systems with fractal-fractional operators. Chaos Solitons Fractals 2019, 123, 320–337. [Google Scholar] [CrossRef]
  12. Liu, Q.; Liu, F.; Turner, I.; Anh, V.; Gu, Y. A RBF meshless approach for modeling a fractal mobile/immobile transport model. Appl. Math. Comput. 2014, 226, 336–347. [Google Scholar] [CrossRef]
  13. Saqib, M.; Khan, I.; Shafie, S. Application of Atangana-Baleanu fractional derivative to MHD channel flow of CMC-based-CNT’s nanofluid through a porous medium. Chaos Solitons Fractals 2018, 116, 79–85. [Google Scholar] [CrossRef]
  14. Podlubny, I. Fractional Differential Equations; Academic Press: San Diego, CA, USA, 1999. [Google Scholar]
  15. Zheng, Z.M.; Li, Z.P.; Xiong, X.T. An improved error bound on the boundary inversion for a sideways heat equation. São Paulo J. Math. Sci. 2020, 14, 287–300. [Google Scholar] [CrossRef]
  16. Qian, Z. Regularization methods for the sideways heat equation and the idea of modifying the “kernel” in the frequency domain. Commun. Appl. Math. Comput. 2012, 26, 298–311. (In Chinese) [Google Scholar]
  17. Carasso, A. Determining surface temperatures from interior observations. SIAM J. Appl. Math. 1982, 42, 558–574. [Google Scholar] [CrossRef]
  18. Eldén, L. Modified equations for approximating the solution of a Cauchy problem for the heat equation. Inverse Ill-Posed Probl. 1987, 4, 345–350. [Google Scholar]
  19. Eldén, L. Approximations for a Cauchy problem for the heat equation. Inverse Probl. 1987, 3, 263–273. [Google Scholar]
  20. Nguyen, H.T.; Luu, V.C.H. Two new regularization methods for solving sideways heat equation. J. Inequal. Appl. 2015, 2015, 1–17. [Google Scholar] [CrossRef] [Green Version]
  21. Wang, J.R. Uniform convergence of wavelet solution to the sideways heat equation. Acta Math. Sin. 2010, 26, 1981–1992. [Google Scholar] [CrossRef]
  22. Qiu, C.Y.; Fu, C.L.; Zhu, Y.B. Wavelets and regularization of the sideways heat equation. Comput. Math. Appl. 2003, 46, 821–829. [Google Scholar] [CrossRef] [Green Version]
  23. Fu, C.L.; Qiu, C.Y. Wavelet and error estimation of surface heat flux. J. Comput. Appl. Math. 2003, 150, 143–155. [Google Scholar]
  24. Seidman, T.I.; Eldén, L. An “optimal filtering” method for the sideways heat equation. Inverse Probl. 1990, 6, 681–696. [Google Scholar] [CrossRef]
  25. Xiong, X.T.; Fu, C.L.; Li, H.F. Fourier regularization method of a sideways heat equation for determining surface heat flux. J. Math. Anal. Appl. 2006, 317, 331–348. [Google Scholar] [CrossRef] [Green Version]
  26. Xiong, X.T.; Fu, C.L.; Li, H.F. Central difference method of a non-standard inverse heat conduction problem for determining surface heat flux from interior observations. Appl. Math. Comput. 2006, 173, 1265–1287. [Google Scholar] [CrossRef]
  27. Eldén, L. Numerical solution of the sideways heat equation. In Inverse Problems in Diffusion Processes; SIAM: Philadelphia, PA, USA, 1995; pp. 130–150. [Google Scholar]
  28. Murio, D.A. The mollification method and the numerical solution of the inverse heat conduction problem by finite differences. Comput. Math. Appl. 1989, 17, 1385–1396. [Google Scholar] [CrossRef] [Green Version]
  29. Huy Tuan, N.; Lesnic, D.; Quoc Viet, T.; Van Au, V. Regularization of semilinear sideways heat equation. IMA J. Appl. Math. 2019, 84, 258–291. [Google Scholar] [CrossRef]
  30. Anh Triet, N.; O’Regan, D.; Baleanu, D.; Hoang Luc, N.; Can, N. A filter method for inverse nonlinear sideways heat equation. Adv. Differ. Equ. 2020, 149, 1–18. [Google Scholar] [CrossRef]
  31. Xiong, X.T.; Guo, H.B.; Liu, X.H. An inverse problem for a fractional diffusion equation. J. Comput. Appl. Math. 2012, 236, 4474–4484. [Google Scholar] [CrossRef]
  32. Xiong, X.T.; Bai, E.P. An optimal filtering method for the sideways fractional heat equation. J. Northwest Norm. Univ. 2020, 56, 14–16, 47. (In Chinese) [Google Scholar]
  33. Li, M.; Xi, X.X.; Xiong, X.T. Regularization for a fractional sideways heat equation. J. Comput. Appl. Math. 2014, 255, 28–43. [Google Scholar] [CrossRef]
  34. Zheng, G.H.; Wei, T. Spectral regularization method for solving a time-fractional inverse diffusion problem. Appl. Math. Comput. 2011, 218, 396–405. [Google Scholar] [CrossRef]
  35. Zheng, G.H.; Wei, T. Spectral regularization method for a Cauchy problem of the time fractional advection-dispersion equation. J. Comput. Appl. Math. 2010, 233, 2631–2640. [Google Scholar] [CrossRef] [Green Version]
  36. Zheng, G.H.; Wei, T. Spectral regularization method for the time fractional inverse advection-dispersion equation. Math. Comput. Simul. 2010, 81, 37–51. [Google Scholar] [CrossRef]
  37. Zhang, H.W.; Zhang, X.J. Tikhonov-type regularization method for a sideways problem of the time-fractional diffusion equation. AIMS Math. 2021, 6, 90–101. [Google Scholar] [CrossRef]
  38. Qian, Z.; Fu, C.L. Regularization strategies for a two-dimensional inverse heat conduction problem. Inverse Probl. 2007, 23, 1053–1068. [Google Scholar] [CrossRef]
  39. Liu, S.S.; Feng, L.X. An Inverse Problem for a Two-Dimensional Time-Fractional Sideways Heat Equation. Math. Probl. Eng. 2020, 2020, 1–13. [Google Scholar] [CrossRef] [Green Version]
  40. Liu, S.S.; Feng, L.X. A revised Tikhonov regularization method for a Cauchy problem of two-dimensional heat conduction equation. Math. Probl. Eng. 2018, 2018, 1–8. [Google Scholar] [CrossRef] [Green Version]
  41. Xiong, X.T.; Xue, X.M. Fractional Tikhonov method for an inverse time-fractional diffusion problem in 2-dimensional space. Bull. Malays. Math. Sci. Soc. 2020, 43, 25–38. [Google Scholar] [CrossRef]
  42. Xiong, X.T.; Zhou, Q.; Hon, Y.C. An inverse problem for fractional diffusion equation in 2-dimensional case: Stability analysis and regularization. J. Math. Anal. Appl. 2012, 393, 185–199. [Google Scholar] [CrossRef] [Green Version]
  43. Guo, L.; Murio, D.A. A mollified space-marching finite-different algorithm for the two-dimensional inverse heat conduction problem with slab symmetry. Inverse Probl. 1991, 7, 247–259. [Google Scholar] [CrossRef]
  44. Liu, C.S.; Chang, C.W. A spring-damping regularization of the Fourier sine series solution to the inverse Cauchy problem for a 3D sideways heat equation. Inverse Probl. Sci. Eng. 2020, 29, 196–219. [Google Scholar] [CrossRef]
  45. Luan, T.N.; Khanh, T.Q. Determination of temperature distribution and thermal flux for two-dimensional inhomogeneous sideways heat equations. Adv. Comput. Math. 2020, 46, 1–28. [Google Scholar] [CrossRef]
  46. Qian, Z.; Fu, C.L.; Xiong, X.T. A modified method for determining the surface heat flux of IHCP. Inverse Probl. Sci. Eng. 2007, 15, 249–265. [Google Scholar] [CrossRef]
Publisher’s Note: MDPI stays neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Share and Cite

MDPI and ACS Style

Chen, Y.; Qiao, Y.; Xiong, X. Regularization for a Sideways Problem of the Non-Homogeneous Fractional Diffusion Equation. Fractal Fract. 2022, 6, 312. https://doi.org/10.3390/fractalfract6060312

AMA Style

Chen Y, Qiao Y, Xiong X. Regularization for a Sideways Problem of the Non-Homogeneous Fractional Diffusion Equation. Fractal and Fractional. 2022; 6(6):312. https://doi.org/10.3390/fractalfract6060312

Chicago/Turabian Style

Chen, Yonggang, Yu Qiao, and Xiangtuan Xiong. 2022. "Regularization for a Sideways Problem of the Non-Homogeneous Fractional Diffusion Equation" Fractal and Fractional 6, no. 6: 312. https://doi.org/10.3390/fractalfract6060312

Article Metrics

Back to TopTop