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Article

The Studies of (Dual) Fusion Frames on Hilbert Space and Generalization of the Index Set

College of Mathematics and Statistics, Tianshui Normal University, Tianshui 741001, China
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Mathematics 2025, 13(19), 3164; https://doi.org/10.3390/math13193164
Submission received: 30 July 2025 / Revised: 21 September 2025 / Accepted: 30 September 2025 / Published: 2 October 2025

Abstract

In this paper, we begin with the classical concept of tight frames in Hilbert spaces. First, we introduce the orthogonal projection P between H and θ ( H ) (the range of the frame transform θ associated with a traditional tight frame) and investigate the relationship between P and θ . We then explore fusion frames and extend the index set to an infinite set through a concrete example. Second, we examine the role of orthogonal projections in fusion frames with particular emphasis on robustness and redundancy illustrated by examples. Finally, we study dual fusion frames and establish several important results, especially concerning the relationship between the frame operators of two types of dual fusion frames.

1. Introduction

Frame theory plays an important role in signal processing, image processing, data compression, sampling theory, and related fields. In 1952, Duffin and Schaeffer [1] introduced the concept of frames in Hilbert spaces in their study of non-harmonic Fourier series. However, this idea initially received little attention. It was not until 1986 that Daubechies, Grossman, and Meyer [2] carried out groundbreaking work in this area, after which frame theory began to be extensively studied.
Casazza and Kutyniok [3] later introduced fusion frames and investigated their properties, perturbations, and the approximation of inverse operators. In recent years, the theory of fusion frames has also undergone rapid development [4,5,6,7]. Fusion frames generalize traditional frames and are particularly well suited for processing block data or multi-channel signals, as they combine orthogonal projections of subspaces with weights.
More recently, considerable attention has been devoted to the study of dual frames. For example, J. Lopez, Han Deguang, Sun Wenchang, and others [8,9,10,11,12,13,14,15,16] have investigated the problem of selecting optimal dual frames from various perspectives. Their contributions have enabled frame theory to achieve significant progress in practical applications.
Orthogonal projection also plays a central role in frame theory. It is fundamental in contexts ranging from rigorous decomposition in Hilbert spaces to efficient approximation in machine learning, and from time-frequency localization in multiresolution analysis to geometric dimensionality reduction in optimization problems. Orthogonal projection provides an indispensable theoretical foundation for the modeling, analysis, and control of complex systems. By balancing redundancy and efficiency through orthogonality constraints, it continues to play a key role in fields such as signal processing, communications, and control [17].
Throughout this paper, H is a Hilbert spaces, we write W = { ( W i , w i ) } i I as W = { ( W i , w i P W i ) } i I in Section 3 for the convenience, and denote f 2 by f , f . The symbol I H denotes the identity operator on H. We now present the preliminary definitions and theorems used in this paper.
Definition 1 
(see [18]). A sequence { f i , i I } for a Hilbert space H is called a frame if there exist constants a , b > 0 such that for any f H ,
a f 2 i I f , f i 2 b f 2 .
The constants a and b are called the lower and the upper frame bounds, respectively. A frame is called tight frame if a = b and a normalized tight frame if a = b = 1 .
Definition 2 
(see [18]). Let { f i , i I } be a frame for a Hilbert space H, and let { e i , i I } be its orthonormal basis. The associated frame transform θ is defined by
θ : H H with θ ( f ) = i I f , f i e i for any f H .
Then θ is adjointable, its adjoint θ * : H H is given by
θ * ( f ) = i I f , e i f i ,
where θ * ( e i ) = f i .
Moreover, we have
S ( f ) = θ * θ ( f ) = θ * i I f , f i e i = i I f , f i θ * ( e i ) = i I f , f i f i .
A direct calculation now yields
S ( f ) , f = i I f , f i f i , f = i I f , f i f i , f .
If { f i , i I } is a frame for a Hilbert space H, then the operator S = θ * θ is a positive, self-adjoint and invertible operator on H, called the frame operator.
It follows from Definition 2 that { f i , i I } is a-tight frame if and only if S = θ * θ = a I H and a normalized tight frame if and only if S = θ * θ = I H .
Since S ( f ) = i I f , f i f i , using S 1 ( f ) to replace f, we obtain
f = S S 1 ( f ) = i I S 1 ( f ) , f i f i = i I f , S 1 ( f i ) f i ,
and
f = S 1 S ( f ) = S 1 i I f , f i f i = i I f , f i S 1 ( f i ) .
Then,
f = i I f , f i S 1 ( f i ) = i I f , S 1 ( f i ) f i .
We now recall the definition of the dual frame.
Definition 3 
(see [18]). Let { f i , i I } be a frame for a Hilbert space H with the frame operator S. Then { S 1 ( f i ) , i I } is called the canonical dual frame of { f i , i I } . If a frame { g i , i I } for H satisfies
i I f , f i g i = i I f , g i f i , for any f H ,
then { g i , i I } is called an alternate dual frame of { f i , i I } .
Definition 4 
(see [19]). Let I be a countable index set, let { W i } i I be a family of closed subspaces of H, and let { w i > 0 } i I be a family of weights. Then W = { ( W i , w i ) } i I is a fusion frame if there exist constants 0 < A < B < + so that
A f , f i I w i P W i ( f ) , w i P W i ( f ) B f , f for any f H ,
where P W i : H W i is the orthogonal projection. The constants A and B are called the lower and the upper fusion frame bounds, respectively.
The family W = { ( W i , w i P W i ) } i I is called A-tight fusion frame if A = B and a parseval fusion frame if A = B = 1 . If only the right-hand inequality holds, it is called a Bessel fusion sequence with Bessel frame bound B. Family W = { ( W i , 1 P W i ) } i I is called 1-consistent Parseval fusion frame if
i I P W i ( f ) , P W i ( f ) = f , f for any f H ,
or w-consistent Parseval fusion frame if
i I w P W i ( f ) , w P W i ( f ) = f , f for any f H .
Theorem 1 
(see [20]). Let H be a Hilbert space, and let { P i } i I be orthogonal projections. If P i ( f ) = f i for any f H , W i = span { f i } ¯ i I . Then { f i , i I } is a frame for H if and only if W = { ( W i , w i ) } i I is fusion frame for H with the frame bounds unchanged and the weight set being w i = f i > 0 .
Theorem 2 
(see [20]). Let { W i } i I be a sequence of closed subspaces of H, { w i > 0 } i I be the weight set, and let { φ i j , j J } be frames for W i . Then W = { ( W i , w i ) } i I is a fusion frame for H if and only if { w i φ i j , i I , j J } is a frame for H.

2. Results

2.1. Discovery of Fusion Frames on Hilbert Spaces and Generalization of the Index Set

Theorem 3. 
Let { f i , i I } be a-tight frame for H with the frame transform θ, and let P : H θ ( H ) be an orthogonal projection. Then P ( e i ) = 1 a θ ( f i ) and θ θ * = a P , where { e i , i I } is the orthonormal basis for H.
Proof. 
Since { f i , i I } is a-tight frame for H, θ * θ = a I H and P = I H on θ ( H ) , i.e., P θ ( H ) = θ ( H ) . Then for any f H ,
θ ( f ) , P ( e i ) = P θ ( f ) , e i = θ ( f ) , e i = f , θ * ( e i ) = f , f i = 1 a θ ( f ) , θ ( f i ) = θ ( f ) , 1 a θ ( f i ) ,
therefore, P ( e i ) = 1 a θ ( f i ) or θ ( f i ) = a P ( e i ) .
Since f = i I f , e i e i , we obtain
θ θ * ( f ) = θ θ * i I f , e i e i = θ i I f , e i θ * ( e i ) = θ i I f , e i f i = i I f , e i θ ( f i ) = i I f , e i a P ( e i ) = a P i I f , e i e i = a P ( f ) .
By the arbitrariness of f, it follows that θ θ * = a P .
In addition, from P = 1 a θ θ * and θ * θ = a I , we have
P 2 = 1 a θ θ * 1 a θ θ * = 1 a 2 θ θ * θ θ * = 1 a 2 θ ( a I ) θ * = 1 a θ θ * = P .
Its self-adjointness is obvious. Thus, P 2 = P = P * , which fully verifies that P acts as an orthogonal projection in the relevant context. □
Let { f i j , i I , j J } be a i -tight frame sequence for H with the frame transforms θ i (where i is the number of frames and j is the dimension of the frames), and let P i : H θ i ( H ) be the orthogonal projections. Then θ i θ i * = a i P i , and
i I ( a i ) 2 P i = i I a i P i = i I θ i θ i * .
Therefore, { ( θ i ( H ) , a i P θ i ( H ) ) } i I is a fusion frame if and only if there exist constants 0 < A < B < + so that
A I H i I ( a i ) 2 P i = i I θ i θ i * B I H .
Obviously, since i I θ i θ i * i I θ i * 2 I H , when I is a finite set, { ( θ i ( H ) , a i P θ i ( H ) ) } i I must be a Bessel fusion sequence.
Our questions are, do such traditional frames and fusion frames exist? And, can I here be extended to an infinite set, i.e., i N + ? Our answers are affirmative and we now give example below.
Example 1. 
Let f i j = a i e j with a i > 0 and i = 1 + a i = s , Then { ( θ i ( H ) , a i P θ i ( H ) ) } i N + is a s-tight fusion frame for H, where { e j , j J } is the standard orthonormal basis for H.
Proof. 
For any f H , we have
j J f , f i j f i j , f = j J f , a i e j a i e j , f = a i j J f , e j e j , f = a i f , f ,
so { f i j , i N + , j J } are a i -tight frames for H. Since
θ i ( f ) = j J f , a i e j e j = a i j J f , e j e j = a i f ,
i.e., θ i = a i I H , θ i * = ( a i I H ) * = a i I H . Then
θ i θ i * = ( a i I H ) ( a i I H ) = a i I H = a i P i ,
which means that P i = I H satisfying P 2 = P = P * and
i = 1 + ( a i ) 2 P i = i = 1 + a i P i = i = 1 + θ i θ i * = i = 1 + a i I H = s I H .
Therefore, { ( θ i ( H ) , a i P θ i ( H ) ) } i N + is a s-tight fusion frame.
However, { ( θ i ( H ) , a i P θ i ( H ) ) } i N + cannot be 1-uniform fusion frame or w-uniform fusion frame, because the constant series i = 1 + w ( w > 0 ) diverges forever unless I is a finite set. □
We present it in the form of a certain theorem.
Theorem 4. 
Let H be a Hilbert space. Then there exists a sequence of a i -tight frames { f i j , i N + , j J } for H such that { ( θ i ( H ) , a i P θ i ( H ) ) } i N + is a tight fusion frame for H, where θ i are the frame transforms of { f i j , i I , j J } , P i : H θ i ( H ) are the orthogonal projections.
Remark 1. 
(1) Example 1 makes use of the convergence of positive-term series. For instance, if we take a i = 1 2 i , then i = 1 + a i = 1 , and { ( θ i ( H ) , a i P θ i ( H ) ) } i N + forms a Parseval fusion frame, and in this case, i = 1 + θ i θ i * = I H .
In fact, for the positive term-series considered here, it is sufficient to establish convergence, there is no need to compute the exact sum. Moreover, many series can only be analyzed in terms of convergence, without an explicit evaluation of their sums. Even in such cases, { ( θ i ( H ) , a i P θ i ( H ) ) } i N + still constitutes a (tight) fusion frame.
(2) The conclusion only holds for traditional tight frames, since the relationship between the frame transform and orthogonal projection exists exclusively in the tight-frame setting.
(3) Example 1 and Theorem 4 establish a close connection between traditional frames and fusion frames, and further realize the closed subspaces W i of H by taking W i = P θ i ( H ) . Even more significantly, the index set I is generalized to infinite sets.

2.2. Orthogonal Projections in the Fusion Frames

The orthogonal projector P is a self-adjoint operator satisfying P 2 = P , i.e., P 2 = P = P * . It projects element of H onto a closed subspace, and the projection is orthogonal to the complement of that subspace, that is, the inner product of the residual with the subspace is zero. Below, we present some simple examples in L 2 ( R ) and L 2 ( [ a , b ] ) .
Example 2. 
In L 2 ( [ a , b ] ) , let M = { c c R } . Then for any f L 2 [ a , b ] and for any x [ a , b ] ,
P M f = 1 b a a b f ( x ) d x .
Example 3. 
In L 2 [ π , π ] , let M n = span { 1 , cos x , sin x , , cos n x , sin n x } . Then
P M n f = a 0 2 + k = 1 n ( a k cos k x + b k sin k x )
for any f L 2 [ π , π ] and for any x [ π , π ] , where the coefficients are the Fourier coefficients.
Example 4. 
In L 2 ( R ) , let I = [ c , d ] be a fixed interval, and let
M = { g g L 2 ( R ) , g ( x ) = 0 , x I } .
Then
P M f = f ( x ) x I 0 x I .
A fusion frame is a subspace frame. Its central role lies in providing stable signal representation and reconstruction through subspace decomposition and weight balancing, while preserving the characteristics of each data source. Fusion frames thus serve as an important theoretical tool in multimodal and multi-sensor data processing. The following examples illustrate the role of orthogonal projection in the fusion frames and in the projection process as a whole.
Example 5. 
Let H = R 2 , W 1 = span { ( 1 , 0 ) } , W 2 = span { ( 0 , 1 ) } (i.e., W 1 is the x-axis and W 2 is the y-axis), v 1 = v 2 = 1 . Then for any f = ( a , b ) R 2 , P W 1 ( f ) = ( a , 0 ) , P W 1 ( f ) 2 = a 2 , P W 2 ( f ) = ( 0 , b ) , P W 2 ( f ) 2 = b 2 . Thus, the weighted sum is
i = 1 2 v i 2 P W i ( f ) 2 = a 2 + b 2 = f 2 .
Therefore, { ( W 1 , 1 ) , ( W 2 , 1 ) } is a Parseval fusion frame.
If W 2 fails, and only W 1 and v 1 are retained, then the weighted sum is a 2 , which cannot control f 2 . However, if a third subspace W 3 = span { ( a , b ) } is added (i.e., W 3 is the line y = b a x ( a 0 )). Let v 3 = 1 , then P W 3 ( f ) = ( a , b ) and the weighted sum is
v 1 2 P W 1 ( f ) 2 + v 3 2 P W 3 ( f ) 2 = a 2 + ( a 2 + b 2 ) .
Since
a 2 + b 2 a 2 + ( a 2 + b 2 ) 2 ( a 2 + b 2 ) ,
f 2 v 1 2 P W 1 ( f ) 2 + v 3 2 P W 3 ( f ) 2 2 f 2 .
Therefore, { ( W 1 , 1 ) , ( W 3 , 1 ) } is a fusion frame, and the lower and upper fusion frame bounds are A = 1 , B = 2 , respectively. In other words, when W 2 fails, f can still be reconstructed through W 1 and W 3 , which demonstrates the robustness of the fusion frame.
In addition, we can also add two subspaces W 4 = span { ( 1 , 1 ) } , W 5 = span { ( 1 , 1 ) } (i.e., W 4 is the line y = x , W 5 is the line y = x ), v 4 = v 5 = 1 . Then,
P W 4 ( f ) = a + b 2 , a + b 2 , P W 5 ( f ) = a b 2 , b a 2 ,
and the weighted sum is
v 1 2 P W 1 ( f ) 2 + v 4 2 P W 4 ( f ) 2 + v 5 2 P W 5 ( f ) 2 = a 2 + ( a + b ) 2 2 + ( a b ) 2 2 = a 2 + ( a 2 + b 2 ) .
Thus,
f 2 v 1 2 P W 1 ( f ) 2 + v 4 2 P W 4 ( f ) 2 + v 5 2 P W 5 ( f ) 2 2 f 2 .
Therefore, { ( W 1 , 1 ) , ( W 4 , 1 ) , ( W 5 , 1 ) } is a fusion frame. In other words, f can still be reconstructed through W 1 , W 4 , and W 5 .
Orthogonal projection is also a fundamental tool for constructing tight frames. For instance, redundant frames can be transformed into Parseval frames by means of orthogonal projection. This property ensures lossless reconstruction in signal processing.
Example 6. 
Let H = R 2 , W 1 = span { ( 1 , 0 ) } , W 2 = span { ( 0 , 1 ) } , W 3 = span { ( 1 , 1 ) } , v 1 = v 2 = v 3 = 1 . Then for any f = ( a , b ) T R 2 , the weighted sum is
f 2 = a 2 + b 2 i = 1 3 v i 2 P W i ( f ) 2 = a 2 + b 2 + ( a + b ) 2 2 2 ( a 2 + b 2 ) = 2 f 2 .
Therefore, { ( W 1 , 1 ) , ( W 2 , 1 ) , ( W 3 , 1 ) } is a fusion frame, but not a Parseval fusion frame.
Since W 3 can be linearly represented by W 1 and W 2 , it is therefore a redundant frame. Next, we transform it into a Parseval frame. we derive the analysis operator T of f. Since
T f = i = 1 3 v i 2 P W i ( f ) = ( a , 0 ) T + ( 0 , b ) T + a + b 2 , a + b 2 T = 3 a + b 2 , a + 3 b 2 T ,
= 3 2 1 2 1 2 3 2 a b = 3 2 1 2 1 2 3 2 f , T = 3 2 1 2 1 2 3 2 .
Thus, T is a symmetric matrix, and
T 1 = 3 4 1 4 1 4 3 4 .
Projecting T 1 f = 3 a b 4 , a 3 b 4 T onto the original subspaces yields
P W 1 ( T 1 f ) = 3 a b 4 , 0 , P W 2 ( T 1 f ) = 0 , a 3 b 4 , P W 3 ( T 1 f ) = a + b 4 , a + b 4 .
After adjusting the weights v 1 = v 2 = 1 , v 3 = 3 , the weighted sum is obtained as
i = 1 3 v i 2 P W i ( T 1 f ) 2 = a 2 + b 2 = f 2 .
Thus, by projecting the subspaces of the redundant frame via T 1 and adjusting the weights, the redundant frame is converted into a Parseval fusion frame.

2.3. Research on Dual Fusion Frames on Hilbert Space

In this section, we begin with an example to explore how traditional dual frames in Hilbert spaces recover original signals in cases of data loss demonstrating the importance and research significance of dual frames.
Example 7. 
Let x 1 = 1 0 , x 2 = 3 2 5 2 , x 3 = 3 2 5 2 . Then θ x = 1 0 3 2 5 2 3 2 5 2 ,
S = θ x * θ x = θ x T θ x = 1 3 2 3 2 0 5 2 5 2 1 0 3 2 5 2 3 2 5 2 = 5 2 0 0 5 2 = 5 2 I ,
so X = { x 1 , x 2 , x 3 } is a tight frame for R 2 with frame bound 5 2 , where θ x is the frame transform of X and S is its frame operator.
Let the original signal vector be x = 1 1 . Then the frame coefficients are c 1 = x , x 1 = x T x 1 = 1 , c 2 = x , x 2 = 3 + 5 2 , c 3 = x , x 3 = 5 3 2 . Suppose that during transmission, the original signal loses c 3 , how can we recover the original signal?
We try to recover it using the alternate dual frame Y = { y 1 , y 2 , y 3 } of X.
Since c 3 is lost, let us set y 3 = 0 0 , y 1 = a b , y 2 = c d . Then θ Y = a b c d 0 0 . Since Y is the alternate dual frame of X, they are mutually alternate dual frames and θ X * θ Y = θ X T θ Y = I or θ Y * θ X = θ Y T θ X = I . Then we have
θ X T θ Y = 1 3 2 3 2 0 5 2 5 2 a b c d 0 0 = 1 0 0 1 .
It is solved that a = 1 , b = 3 5 , c = 0 , d = 2 5 . So y 1 = 1 3 5 , y 2 = 0 2 5 , y 3 = 0 0 , and
c 1 y 1 + c 2 y 2 = 1 1 3 5 + 3 + 5 2 0 2 5 = 1 1 = x .
i.e., the alternate dual frame Y of X can recover the original signal.
The canonical dual frame Z = { z 1 , z 2 , z 3 } of X can also recover the original signal.
Since S x = 5 2 I , S x 1 = 2 5 I . Then we obtain
z 1 = S 1 ( x 1 ) = 2 5 I 1 0 = 2 5 0 , z 2 = S 1 ( x 2 ) = 2 5 I 3 2 5 2 = 3 5 5 5 ,
z 3 = S 1 ( x 3 ) = 2 5 I 3 2 5 2 = 3 5 5 5 .
Taking
c 1 = x , z 1 = x T z 1 = 2 5 , c 2 = x , z 2 = x T z 2 = 3 + 5 5 ,
c 3 = x , z 3 = x T z 3 = 5 3 5 ,
then
c 1 x 1 + c 2 x 2 + c 3 x 3 = 2 5 1 0 3 + 5 5 3 2 5 2 + 5 3 5 3 2 5 2 = 1 1 = x .
This means that the canonical dual frame Z of X can also recover the original signal.
Meanwhile, let y i = z i + u i ( i = 1 , 2 , 3 ). Then
u 1 = 3 5 3 5 , u 2 = 3 5 1 5 , u 3 = 3 5 1 5 ,
and
c 1 u 1 + c 2 u 2 + c 3 u 3 = 1 3 5 3 5 + 3 + 5 2 3 5 1 5 + 5 3 2 3 5 1 5 = 0 0 .
We obtain i = 1 3 x , x i u i = 0 , i.e., θ x * θ u = 0 , and of course θ u * θ x = 0 , where U = { u 1 , u 2 , u 3 } .
It follows that the frames X and U are disjointed, meaning that any alternate dual frame of a frame can be expressed as the sum of its canonical dual frame and a frame can disjoint from itself, and the canonical dual frame is the “minimal” dual frame.
Next, we study dual fusion frames on Hilbert spaces.
Definition 5 
(see [19]). Let W = { ( W i , w i P W i ) } i I be a fusion frame for H, the analysis operator is defined by
T : H i I W i 2 with T ( f ) = { w i P W i ( f ) } i I for any f H ,
where i I W i 2 = { f i } i I f i W i and { f i W i } i I 2 ( I ) . It can easily be shown that the synthesis operator T * , which is defined to be the adjoint operator, is given by
T * : i I W i 2 H with T * ( { f i } ) = i I w i P W i ( f i ) for any { f i } i I W i 2 .
The fusion frame operator S for W = { ( W i , w i P W i ) } i I is defined by
S : H H with S ( f ) = T * T ( f ) = i I w i 2 P W i ( f ) .
If W = { ( W i , w i P W i ) } i I be a fusion frame for H with fusion frame bound A and B, then the associated fusion frame operator S is a self-adjoint, positive, and invertible operator on H, and A I H S = i I w i 2 P W i B I H .
It follows from Definition 5 that W = { ( W i , w i P W i ) } i I is a B-tight fusion frame if and only if S = B I H , and is a Parseval fusion frame if and only if S = I H .
Obviously, if W = { ( W i , w i P W i ) } i I is a fusion frame for H with fusion frame operator S, then { ( W i , w i P W i S 1 / 2 ) } i I is a Parseval fusion frame for H. In fact,
i I w i 2 ( P W i S 1 / 2 ) ( P W i S 1 / 2 ) = S 1 / 2 i I w i 2 P W i S 1 / 2 = S 1 / 2 S S 1 / 2 = I H .
Theorem 5 
(see [1]). Let T be a bounded linear operator on H, and let V be a closed subspace of H. Then P V T * = P V T * P T ( V ) ¯ . Moreover if T is a unitary operator, then P T ( V ) ¯ T = T P V , where P is the orthogonal projection from H to V.
It follows from Theorem 5 that ( P V T * ) * = ( P V T * P T ( V ) ¯ ) * , i.e., T P V = P T ( V ) ¯ T P V . So, if W = { ( W i , w i P W i ) } i I is the fusion frame with fusion frame operator S, then
S 1 P W i = P S 1 ( W i ) S 1 P W i .
Therefore, for any f H , S ( f ) = i I w i 2 P W i ( f ) , and
f = S 1 S ( f ) = i I w i 2 S 1 P W i ( f ) = i I w i 2 P S 1 ( W i ) S 1 P W i ( f ) .
S 1 ( W ) = { ( S 1 ( W i ) , w i P S 1 ( W i ) ) } i I is called the canonical dual fusion frame of W = { ( W i , w i P W i ) } i I .
Corollary 1. 
Let W = { ( W i , w i P W i ) } i I be the fusion frame for H with fusion frame operator S, and let S 1 ( W ) = { ( S 1 ( W i ) , w i P S 1 ( W i ) ) } i I be its the canonical dual fusion frame. Then S S 1 ( W ) = S 1 .
Proof. 
For any f H ,
S S 1 ( W ) ( f ) = i I w i 2 P S 1 ( W i ) S 1 P W i ( f ) = S 1 i I w i 2 P W i S 1 ( f ) = S 1 S S 1 ( f ) = S 1 ( f ) .
Therefore, the frame operator of the canonical dual fusion frame is the inverse of its own frame operator. It is obvious that if W = { ( W i , w i P W i ) } i I is a parseval fusion frame, i.e., S = I H , then its canonical dual fusion frame is itself. □
Definition 6 
(see [16]). Let W = { ( W i , w i P W i ) } i I and V = { ( V i , v i Q V i ) } i I be fusion frames for H. If for any f H ,
f = i I w i v i Q V i S 1 P W i ( f ) ,
then V = { ( V i , v i Q V i ) } i I is called an alternate dual fusion frame of W = { ( W i , w i P W i ) } i I , where S is the fusion frame operator of W = { ( W i , w i P W i ) } i I .
Remark 2. 
(1) The canonical dual fusion frame of W = { ( W i , w i P W i ) } i I must be its alternate dual fusion frame. In particular, when V i = S 1 ( W i ) and v i = w i , these two dual fusion frames are the same fusion frame.
(2) Traditional alternate dual frames are mutual alternate duals, while alternate dual fusion frames are not dual to each other.
In fact, if V = { ( V i , v i Q V i ) } i I is the alternate dual fusion frame of W = { ( W i , w i P W i ) } i I , then f = i I w i v i Q V i S 1 1 P W i ( f ) for any f H , where S 1 is the fusion frame operator of W = { ( W i , w i P W i ) } i I . If W = { ( W i , w i P W i ) } i I is an alternate dual fusion frame of V = { ( V i , v i Q V i ) } i I , then f = i I w i v i P W i S 2 1 Q V i ( f ) for any f H , where S 2 is the fusion frame operator of V = { ( V i , v i Q V i ) } i I .
In particular, if S 1 = S 2 = S , then the alternate dual fusion frames are mutual alternate duals.
The following are the necessary and sufficient conditions under which they are mutual alternate duals and their stability.
Theorem 6. 
Let W = { ( W i , w i P W i ) } i I and V = { ( V i , v i Q V i ) } i I be fusion frames for H, let T 1 and T 2 be their analysis operators respectively, let T 1 * and T 2 * be their synthesis operators, respectively, and let S 1 and S 2 be their frame operators respectively. Then
(1) W = { ( W i , w i P W i ) } i I and V = { ( V i , v i Q V i ) } i I are mutual alternate duals if and only if T 2 * S 1 1 T 1 = T 1 * S 2 1 T 2 = I H .
(2) If S 1 = S 2 = S and V = { ( V i , v i Q V i ) } i I is alternate dual fusion frames of W = { ( W i , w i P W i ) } i I , then W + V = { ( W i + V i , w i S 1 P W i + v i S 1 Q V i ) } i I is also a fusion frame for H.
Proof. 
(1) For any f H , we have
T 2 * S 1 1 T 1 ( f ) = T 2 * S 1 1 { ( w i P W i ( f ) ) } i I = i I v i Q V i S 1 1 w i P W i ( f ) = i I w i v i Q V i S 1 1 P W i ( f ) ,
T 1 * S 2 1 T 2 ( f ) = T 1 * S 2 1 { ( v i Q V i ( f ) ) } i I = i I w i P W i S 2 1 v i Q V i ( f ) = i I w i v i P W i S 2 1 Q V i ( f ) .
Therefore, W = { ( W i , w i P W i ) } i I and V = { ( V i , v i Q V i ) } i I are mutual alternate duals if and only if
f = i I w i v i Q V i S 1 1 P W i ( f ) = i I w i v i P W i S 2 1 Q V i ( f )
if and only if
f = T 2 * S 1 1 T 1 ( f ) = T 1 * S 2 1 T 2 ( f ) ,
by the arbitrariness of f, we obtain T 2 * S 1 1 T 1 = T 1 * S 2 1 T 2 = I H .
(2) Since S 1 = S 2 = S , W = { ( W i , w i P W i ) } i I and V = { ( V i , v i Q V i ) } i I are mutual alternate duals. Combining with (1) of Theorem 6, for any f H , we have
T 2 * S 1 T 1 ( f ) = i I w i v i Q V i S 1 P W i ( f ) = f , T 1 * S 1 T 2 ( f ) = i I w i v i P W i S 1 Q V i ( f ) = f .
And
T 1 * S 1 T 1 ( f ) = i I w i 2 P W i S 1 P W i ( f ) , T 2 * S 1 T 2 ( f ) = i I v i 2 Q V i S 1 Q V i ( f ) .
Therefore,
i I ( w i S 1 / 2 P W i + v i S 1 / 2 Q V i ) ( f ) , ( w i S 1 / 2 P W i + v i S 1 / 2 Q V i ) ( f ) = i I w i S 1 / 2 P W i ( f ) , w i S 1 / 2 P W i ( f ) + i I w i S 1 / 2 P W i ( f ) , v i S 1 / 2 Q V i ( f ) + i I v i S 1 / 2 Q V i ( f ) , w i S 1 / 2 P W i ( f ) + i I v i S 1 / 2 Q V i ( f ) , v i S 1 / 2 Q V i ( f ) = i I w i 2 P W i S 1 P W i ( f ) , f + i I w i v i Q V i S 1 P W i ( f ) , f + i I w i v i P W i S 1 Q V i ( f ) , f + i I v i 2 Q V i S 1 Q V i ( f ) , f = T 1 * S 1 T 1 ( f ) , f + T 2 * S 1 T 1 ( f ) , f + T 1 * S 1 T 2 ( f ) , f + T 2 * S 1 T 2 ( f ) , f = T 1 * S 1 T 1 ( f ) , f + f , f + f , f + T 2 * S 1 T 2 ( f ) , f = ( T 1 * S 1 T 1 + T 2 * S 1 T 2 + 2 I H ) ( f ) , f ,
that is to say,
i I ( w i S 1 / 2 P W i + v i S 1 / 2 Q V i ) * ( w i S 1 / 2 P W i + v i S 1 / 2 Q V i ) = T 1 * S 1 T 1 + T 2 * S 1 T 2 + 2 I H .
Moreover, since W = { ( W i , w i P W i ) } i I and V = { ( V i , v i Q V i ) } i I are fusion frames for H, there exist constants 0 < A < B < + such that A I H S 1 = S 2 = S B I H . Therefore,
1 B I H S 1 1 A I H ,
and
A B I H 1 B S = 1 B T 1 * T 1 T 1 * S 1 T 1 1 A T 1 * T 1 = 1 A S B A I H .
Similarly, since
A B I H T 2 * S 1 T 2 B A I H ,
we have
2 A B + 1 I H T 1 * S 1 T 1 + T 2 * S 1 T 2 + 2 I H 2 B A + 1 I H ,
so W + V = { ( W i + V i , w i S 1 P W i + v i S 1 Q V i ) } i I is also a fusion frame with frame operator S W + V = T 1 * S 1 T 1 + T 2 * S 1 T 2 + 2 I H and 2 A B + 1 I H S W + V 2 B A + 1 I H . □
Theorem 7. 
Let W = { ( W i , w i P W i ) } i I be a fusion frame for H with fusion frame operator S 1 , let S 1 1 ( W ) = { ( S 1 1 ( W i ) , w i P S 1 1 ( W i ) ) } i I and V = { ( V i , v i Q V i ) } i I be its canonical dual fusion frame and alternate dual fusion frame respectively. Then S 1 1 S 1 1 2 S 2 , where S 2 is the fusion frame operator of V = { ( V i , v i Q V i ) } i I .
Proof. 
Since for any f H ,
i I w i 2 P S 1 1 ( W i ) S 1 1 P W i ( f ) = f = i I w i v i Q V i S 1 1 P W i ( f ) ,
and
i I w i 2 P S 1 1 ( W i ) S 1 1 P W i ( f ) = i I w i 2 S 1 1 P W i ( f ) ,
we have
i I w i 2 S 1 1 P W i ( f ) = f = i I w i v i Q V i S 1 1 P W i ( f ) .
Replacing f with S 1 1 ( f ) ,
i I w i 2 S 1 1 P W i ( S 1 1 ( f ) ) = S 1 1 ( f ) = i I w i v i Q V i S 1 1 P W i ( S 1 1 ( f ) ) .
Therefore,
f , S 1 1 ( f ) = f , i I w i v i Q V i S 1 1 P W i ( S 1 1 ( f ) ) = f , i I w i 2 S 1 1 P W i ( S 1 1 ( f ) ) ,
and
i I v i S 1 1 Q V i ( f ) , w i P W i S 1 1 ( f ) = i I w i P W i S 1 1 ( f ) , w i P W i S 1 1 ( f ) ,
that is to say,
i I v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) , w i P W i S 1 1 ( f ) = 0 .
Moreover, since
i I v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) , v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) 0 ,
we obtain
i I v i S 1 1 Q V i ( f ) , v i S 1 1 Q V i ( f ) = i I v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) + w i P W i S 1 1 ( f ) , v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) + w i P W i S 1 1 ( f ) = i I v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) , v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) + i I v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) , w i P W i S 1 1 ( f ) + i I w i P W i S 1 1 ( f ) , v i S 1 1 Q V i ( f ) w i P W i S 1 1 ( f ) + i I w i P W i S 1 1 ( f ) , w i P W i S 1 1 ( f ) i I w i P W i S 1 1 ( f ) , w i P W i S 1 1 ( f ) .
Thus,
i I w i P W i S 1 1 ( f ) , w i P W i S 1 1 ( f ) i I v i S 1 1 Q V i ( f ) , v i S 1 1 Q V i ( f ) = S 1 1 i I v i 2 Q V i S 1 1 ( f ) , f = S 1 1 S 2 S 1 1 ( f ) , f .
Furthermore, we have
i I w i 2 P W i S 1 1 ( f ) 2 S 1 1 2 S 2 ( f ) , f .
And
i I w i 2 P W i S 1 1 ( f ) 2 = S 1 1 i I w i 2 P W i S 1 1 ( f ) , f = S 1 1 S 1 S 1 1 ( f ) , f = S 1 1 ( f ) , f ,
therefore,
S 1 1 ( f ) , f S 1 1 2 S 2 ( f ) , f .
Since S 1 1 is the frame operator of the canonical dual fusion frame of W = { ( W i , w i P W i ) } i I , Theorem 7 reveals the relationship between the canonical dual fusion frame and the alternate dual fusion frame, especially the relationship between their respective fusion frame operators. □

3. Conclusions

In this paper, we first uncover implicit fusion frames by studying the frame transform and orthogonal projection of traditional tight frames. Next, we present an example connecting traditional tight frames and fusion frames by combining the convergence of positive-term series in mathematical analysis with the orthonormal basis of a Hilbert space. In this context, the index set is extended to an infinite set and both types of frames are explicitly realized. Secondly, we investigated orthogonal projections in fusion frames, particularly their applications in transforming redundant fusion frames into Parseval fusion frames. Finally, we studied the dual fusion frames. Since alternate dual fusion frames are not dual to each other, we first established the necessary and sufficient conditions under which they are mutual alternate duals, and then examined their stability as well as the relationship between the two types of dual fusion frames.

Author Contributions

Writing—original draft, F.D.; Writing—review and editing, F.D.; formal analysis, R.P. All authors have read and agreed to the published version of the manuscript.

Funding

This work is supported by the National Natural Science Foundation of China (No. 11661070).

Data Availability Statement

The original contributions presented in this study are included in the article. Further inquiries can be directed to the corresponding author.

Acknowledgments

We thank two anonymous referees for their comments to improve the manuscript.

Conflicts of Interest

The authors declare no conflicts of interest.

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Dong, F.; Pei, R. The Studies of (Dual) Fusion Frames on Hilbert Space and Generalization of the Index Set. Mathematics 2025, 13, 3164. https://doi.org/10.3390/math13193164

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Dong F, Pei R. The Studies of (Dual) Fusion Frames on Hilbert Space and Generalization of the Index Set. Mathematics. 2025; 13(19):3164. https://doi.org/10.3390/math13193164

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Dong, Fangfang, and Ruichang Pei. 2025. "The Studies of (Dual) Fusion Frames on Hilbert Space and Generalization of the Index Set" Mathematics 13, no. 19: 3164. https://doi.org/10.3390/math13193164

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Dong, F., & Pei, R. (2025). The Studies of (Dual) Fusion Frames on Hilbert Space and Generalization of the Index Set. Mathematics, 13(19), 3164. https://doi.org/10.3390/math13193164

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