2017
DOI: 10.1109/taes.2017.2667899
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Obtaining JTF-Signature of Space-Debris From Incomplete and Phase-Corrupted Data

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Cited by 26 publications
(11 citation statements)
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“…Initialize ρ > 0, Z (0) , and B (0) ; 2. For n = 1 : N Update X (n) by (10); Update Z (n) by (13); Update B (n) by ( 12); End 3. Output X (N+1) by (10).…”
Section: Pnp 2d Admm Methodsmentioning
confidence: 99%
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“…Initialize ρ > 0, Z (0) , and B (0) ; 2. For n = 1 : N Update X (n) by (10); Update Z (n) by (13); Update B (n) by ( 12); End 3. Output X (N+1) by (10).…”
Section: Pnp 2d Admm Methodsmentioning
confidence: 99%
“…Typically, one stage consists of three layers, i.e., the reconstruction layer R •, •, •; ρ (n) ; the denoising layer D •, •; w (n) , where w is the network parameter; and the multiplier update layer U •, •, •; η (n) . The three layers correspond to (10), (13), and (12), respectively. In addition, (•) represents the inputs of each layer.…”
Section: Structure Of Panmentioning
confidence: 99%
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“…With growing scientific research and commercial applications in space, more and more malfunctioning satellites and space debris are occupying precious orbital resources which will bring a great threat to the safety of on-orbit spacecrafts [1,2]. In order to utilize or remove them, space robots have been studied and developed for many years [3].…”
Section: Introductionmentioning
confidence: 99%
“…The l 0 -norm optimization, e.g., orthogonal MP (OMP) [8] and smoothed l 0 -norm method [9], cannot guarantee that the solution is sparsest and may converge to the local minima. The l 1norm optimization, e.g., the fast iterative shrinkage-thresholding algorithm (FISTA) [10,11] and alternating direction method of multipliers (ADMM) [12,13], is the convex approximation of the l 0 -norm [14]. However, the regularization parameter directly affects the performance and how to determine its optimum value remains an open problem [4].…”
Section: Introductionmentioning
confidence: 99%