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Search Results (1,126)

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20 pages, 96432 KiB  
Article
Contrastive Feature Disentanglement via Physical Priors for Underwater Image Enhancement
by Fei Li, Li Wan, Jiangbin Zheng, Lu Wang and Yue Xi
Remote Sens. 2025, 17(5), 759; https://doi.org/10.3390/rs17050759 (registering DOI) - 22 Feb 2025
Viewed by 84
Abstract
Underwater image enhancement (UIE) serves as a fundamental preprocessing step in ocean remote sensing applications, encompassing marine life detection, archaeological surveying, and subsea resource exploration. However, UIE encounters substantial technical challenges due to the intricate physics of underwater light propagation and the inherent [...] Read more.
Underwater image enhancement (UIE) serves as a fundamental preprocessing step in ocean remote sensing applications, encompassing marine life detection, archaeological surveying, and subsea resource exploration. However, UIE encounters substantial technical challenges due to the intricate physics of underwater light propagation and the inherent homogeneity of aquatic environments. Images captured underwater are significantly degraded through wavelength-dependent absorption and scattering processes, resulting in color distortion, contrast degradation, and illumination irregularities. To address these challenges, we propose a contrastive feature disentanglement network (CFD-Net) that systematically addresses underwater image degradation. Our framework employs a multi-stream decomposition architecture with three specialized decoders to disentangle the latent feature space into components associated with degradation and those representing high-quality features. We incorporate hierarchical contrastive learning mechanisms to establish clear relationships between standard and degraded feature spaces, emphasizing intra-layer similarity and inter-layer exclusivity. Through the synergistic utilization of internal feature consistency and cross-component distinctiveness, our framework achieves robust feature extraction without explicit supervision. Compared to existing methods, our approach achieves a 12% higher UIQM score on the EUVP dataset and outperforms other state-of-the-art techniques on various evaluation metrics such as UCIQE, MUSIQ, and NIQE, both quantitatively and qualitatively. Full article
(This article belongs to the Special Issue Ocean Remote Sensing Based on Radar, Sonar and Optical Techniques)
21 pages, 5841 KiB  
Article
Archaeological Ceramic Fabric Attribution Through Material Characterisation—A Case-Study from Vale Pincel I (Sines, Portugal)
by Ana S. Saraiva, Mathilda L. Coutinho, Carlos Tavares da Silva, Joaquina Soares, Susana Duarte and João Pedro Veiga
Heritage 2025, 8(3), 84; https://doi.org/10.3390/heritage8030084 - 20 Feb 2025
Viewed by 150
Abstract
Defining groups of ceramic objects from archaeological excavations is a crucial and primary practice in the study of settlements, providing information related to ceramic technology, provenance, and interactions, among others. This process begins with a macroscopic analysis of each fragment, identifying common features [...] Read more.
Defining groups of ceramic objects from archaeological excavations is a crucial and primary practice in the study of settlements, providing information related to ceramic technology, provenance, and interactions, among others. This process begins with a macroscopic analysis of each fragment, identifying common features to define ceramic fabrics. Regularly, this procedure requires further analytical techniques to refine the attribution of each ceramic object to the corresponding fabric. The Early Neolithic site of Vale Pincel I in Sines, Portugal, dates to the second and third quarters of the sixth millennium BC. The earliest examples of ceramica impressa, described by patterned impressions on the surface (impresso pottery), in Portugal were found here. These artifacts are indicative of the Western Mediterranean Basin cycle pre-Cardial ceramic tradition. From the numerous Neolithic ceramic fragments discovered at Vale Pincel I, archaeologists identified 42 fragments, categorizing them into 2 main groups (A and B) through visual analysis, while a third group (C) remained unclassified. Group A, thick ceramic body with reddish hues and very friable surfaces; Group B, thin ceramic body with greyish to black shades and a cohesive appearance. With the aim to resolve the classification of group C ceramics, this study uses a multi-analytical methodology, combining Optical Microscopy (OM), Wavelength Dispersive X-Ray Fluorescence Spectroscopy (WD-XRF), and X‑Ray Diffraction (XRD). Integrating the analytical data with previously obtained archaeological information, Group C fragments were attributed to Groups A and B, demonstrating the absence of a distinct third group in Vale Pincel I, highlighting the effectiveness of analytical techniques in ceramic studies, and contributing to a deeper understanding of Neolithic ceramic technology in the Western Mediterranean Basin. Full article
20 pages, 7029 KiB  
Article
Tracking of Low Radar Cross-Section Super-Sonic Objects Using Millimeter Wavelength Doppler Radar and Adaptive Digital Signal Processing
by Yair Richter, Shlomo Zach, Maxi Y. Blum, Gad A. Pinhasi and Yosef Pinhasi
Remote Sens. 2025, 17(4), 650; https://doi.org/10.3390/rs17040650 - 14 Feb 2025
Viewed by 306
Abstract
Small targets with low radar cross-section (RCS) and high velocities are very hard to track by radar as long as the frequent variations in speed and location demand shorten the integration temporal window. In this paper, we propose a technique for tracking evasive [...] Read more.
Small targets with low radar cross-section (RCS) and high velocities are very hard to track by radar as long as the frequent variations in speed and location demand shorten the integration temporal window. In this paper, we propose a technique for tracking evasive targets using a continuous wave (CW) radar array of multiple transmitters operating in the millimeter wavelength (MMW). The scheme is demonstrated to detect supersonic moving objects, such as rifle projectiles, with extremely short integration times while utilizing an adaptive processing algorithm of the received signal. Operation at extremely high frequencies qualifies spatial discrimination, leading to resolution improvement over radars operating in commonly used lower frequencies. CW transmissions result in efficient average power utilization and consumption of narrow bandwidths. It is shown that although CW radars are not naturally designed to estimate distances, the array arrangement can track the instantaneous location and velocity of even supersonic targets. Since a CW radar measures the target velocity via the Doppler frequency shift, it is resistant to the detection of undesired immovable objects in multi-scattering scenarios; thus, the tracking ability is not impaired in a stationary, cluttered environment. Using the presented radar scheme is shown to enable the processing of extremely weak signals that are reflected from objects with a low RCS. In the presented approach, the significant improvement in resolution is beneficial for the reduction in the required detection time. In addition, in relation to reducing the target recording time for processing, the presented scheme stimulates the detection and tracking of objects that make frequent changes in their velocity and position. Full article
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<p>Doppler radar system scheme.</p>
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<p>Multi-transmitters—single-receiver Doppler radar system.</p>
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<p>A scale model for a radar system to detect velocity components.</p>
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<p>Velocity resolution <math display="inline"><semantics> <mrow> <mo>∆</mo> <msub> <mrow> <mi mathvariant="normal">v</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math> vs. integration time <math display="inline"><semantics> <mrow> <mi mathvariant="normal">T</mi> <mo>/</mo> <msub> <mrow> <mi mathvariant="normal">T</mi> </mrow> <mrow> <mi mathvariant="normal">o</mi> <mi mathvariant="normal">p</mi> <mi mathvariant="normal">t</mi> </mrow> </msub> </mrow> </semantics></math> as a result of the trade-off between measurement resolution improvement and frequency broadening by data overabundance.</p>
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<p>Resolution vs. integration time over different transmission frequencies of the radar, with the same acceleration <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> <mo>=</mo> <mn>100</mn> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mi mathvariant="normal">m</mi> </mrow> <mrow> <msup> <mrow> <mi mathvariant="normal">s</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msup> </mrow> </mfrac> </mstyle> </mrow> </semantics></math>.</p>
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<p>Locations of the systems used during the experiment. The radar system was placed alongside the bullet’s expected trajectory.</p>
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<p>The radar system used in the experiment; (<b>a</b>) the master unit and (<b>b</b>) the slave unit. *Multiplier: QMM-9940615060.</p>
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<p>Diagram of the measurement performed in the range. The red line is the illustrated trajectory of the measured object. The blue beam and the green beam are the illustrated beams of the antennas.</p>
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<p>Spectral-time representation of the recording from the radar. Two frequencies are obtained at any time slot and transferred to velocity by <math display="inline"><semantics> <mrow> <mi mathvariant="normal">v</mi> <mo>=</mo> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mo>λ</mo> </mrow> <mrow> <mn>2</mn> </mrow> </mfrac> </mstyle> <mi mathvariant="normal">f</mi> </mrow> </semantics></math>.</p>
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<p>Spectral-time representation of the recording from the radar as presented in <a href="#remotesensing-17-00650-f009" class="html-fig">Figure 9</a>, with additional analysis of velocity components extracting.</p>
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<p>Optimal integration times for each velocity component separately over time.</p>
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<p>Spectrogram calculations optimized for the acceleration of the target and extraction of high-quality velocity components. The spectrogram in (<b>a</b>) shows an optimal spectrogram creation process for the upper-velocity component; compared with (<b>b</b>)<b>,</b> it provides earlier data regarding the target that moves towards the radar. The spectrogram in (<b>b</b>) shows an optimal result for the lower velocity component when the graph is narrower and, therefore, shows greater accuracy than the spectrogram from (<b>a</b>). The velocity components were extracted after generating optimal spectrograms, with the upper-velocity component in (<b>c</b>) extracted from the spectrogram in (<b>a</b>) and the velocity component in (<b>d</b>) extracted from the spectrogram in (<b>b</b>).</p>
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<p>Distance calculation from the radar measurements and the estimated distance from the moment of receiving the trigger at 40 ms.</p>
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18 pages, 1807 KiB  
Article
3DVT: Hyperspectral Image Classification Using 3D Dilated Convolution and Mean Transformer
by Xinling Su and Jingbo Shao
Photonics 2025, 12(2), 146; https://doi.org/10.3390/photonics12020146 - 11 Feb 2025
Viewed by 391
Abstract
Hyperspectral imaging and laser technology both rely on different wavelengths of light to analyze the characteristics of materials, revealing their composition, state, or structure through precise spectral data. In hyperspectral image (HSI) classification tasks, the limited number of labeled samples and the lack [...] Read more.
Hyperspectral imaging and laser technology both rely on different wavelengths of light to analyze the characteristics of materials, revealing their composition, state, or structure through precise spectral data. In hyperspectral image (HSI) classification tasks, the limited number of labeled samples and the lack of feature extraction diversity often lead to suboptimal classification performance. Furthermore, traditional convolutional neural networks (CNNs) primarily focus on local features in hyperspectral data, neglecting long-range dependencies and global context. To address these challenges, this paper proposes a novel model that combines CNNs with an average pooling Vision Transformer (ViT) for hyperspectral image classification. The model utilizes three-dimensional dilated convolution and two-dimensional convolution to extract multi-scale spatial–spectral features, while ViT was employed to capture global features and long-range dependencies in the hyperspectral data. Unlike the traditional ViT encoder, which uses linear projection, our model replaces it with average pooling projection. This change enhances the extraction of local features and compensates for the ViT encoder’s limitations in local feature extraction. This hybrid approach effectively combines the local feature extraction strengths of CNNs with the long-range dependency handling capabilities of Transformers, significantly improving overall performance in hyperspectral image classification tasks. Additionally, the proposed method holds promise for the classification of fiber laser spectra, where high precision and spectral analysis are crucial for distinguishing between different fiber laser characteristics. Experimental results demonstrate that the CNN-Transformer model substantially improves classification accuracy on three benchmark hyperspectral datasets. The overall accuracies achieved on the three public datasets—IP, PU, and SV—were 99.35%, 99.31%, and 99.66%, respectively. These advancements offer potential benefits for a wide range of applications, including high-performance optical fiber sensing, laser medicine, and environmental monitoring, where accurate spectral classification is essential for the development of advanced systems in fields such as laser medicine and optical fiber technology. Full article
(This article belongs to the Special Issue Advanced Fiber Laser Technology and Its Application)
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<p>Overall framework of the 3DVT network model.</p>
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<p>ViT encoder with average pooling projection.</p>
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20 pages, 1645 KiB  
Review
Evolution of Light-Sensitive Proteins in Optogenetic Approaches for Vision Restoration: A Comprehensive Review
by Kamil Poboży, Tomasz Poboży, Paweł Domański, Michał Derczyński, Wojciech Konarski and Julia Domańska-Poboża
Biomedicines 2025, 13(2), 429; https://doi.org/10.3390/biomedicines13020429 - 10 Feb 2025
Viewed by 403
Abstract
Retinal degenerations, such as age-related macular degeneration and retinitis pigmentosa, present significant challenges due to genetic heterogeneity, limited therapeutic options, and the progressive loss of photoreceptors in advanced stages. These challenges are compounded by difficulties in precisely targeting residual retinal neurons and ensuring [...] Read more.
Retinal degenerations, such as age-related macular degeneration and retinitis pigmentosa, present significant challenges due to genetic heterogeneity, limited therapeutic options, and the progressive loss of photoreceptors in advanced stages. These challenges are compounded by difficulties in precisely targeting residual retinal neurons and ensuring the sustained efficacy of interventions. Optogenetics offers a novel approach to vision restoration by inducing light sensitivity in residual retinal neurons through gene delivery of light-sensitive opsins. This review traces the evolution of opsins in optogenetic therapies, highlighting advancements from early research on channelrhodopsin-2 (ChR2) to engineered variants addressing key limitations. Red-shifted opsins, including ReaChR and ChrimsonR, reduced phototoxicity by enabling activation under longer wavelengths, while Chronos introduced superior temporal kinetics for dynamic visual tracking. Further innovations, such as Multi-Characteristic Opsin 1 (MCO1), optimized opsin performance under ambient light, bridging the gap to real-world applications. Key milestones include the first partial vision restoration in a human patient using ChrimsonR with light-amplifying goggles and ongoing clinical trials exploring the efficacy of opsin-based therapies for advanced retinal degeneration. While significant progress has been made, challenges remain in achieving sufficient light sensitivity for functional vision under normal ambient lighting conditions in a manner that is both effective and safe, eliminating the need for external light-enhancing devices. As research progresses, optogenetic therapies are positioned to redefine the management of retinal degenerative diseases, offering new hope for millions affected by vision loss. Full article
(This article belongs to the Section Cell Biology and Pathology)
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<p>Schematic illustration of optogenetic vision restoration.</p>
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<p>Chronological order of opsins used in optogenetic vision restoration, arranged according to the date of their first description.</p>
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<p>The activation range and optimal wavelength for the activation of individual opsins.</p>
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14 pages, 749 KiB  
Article
Modelling of X-Ray Spectra Originating from the He- and Li-like Ni Ions for Plasma Electron Temperature Diagnostics Purposes
by Karol Kozioł, Andrzej Brosławski and Jacek Rzadkiewicz
Atoms 2025, 13(2), 18; https://doi.org/10.3390/atoms13020018 - 9 Feb 2025
Viewed by 289
Abstract
The multi-configurational Dirac–Hartree–Fock method has been used to examine the electron correlation effect on wavelengths and transition rates for LK transitions occurring in He- and Li-like nickel ions. The collisional-radiative modelling approach has been used to simulate the X-ray spectra, in [...] Read more.
The multi-configurational Dirac–Hartree–Fock method has been used to examine the electron correlation effect on wavelengths and transition rates for LK transitions occurring in He- and Li-like nickel ions. The collisional-radiative modelling approach has been used to simulate the X-ray spectra, in a 1.585–1.620 Å wavelength range, originating from the He-like nickel ions and their dielectronic Li-, Be-, and B-like satellites for various electron temperature values in the 2 keV to 8 keV range. The presented results may be useful in improving the plasma electron temperature diagnostics based on nickel spectra. Full article
(This article belongs to the Special Issue Atom and Plasma Spectroscopy)
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<p>Convergence of CI calculations for transition energies in He-like Ni.</p>
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<p>Convergence of CI calculations for transition energies in Li-like Ni.</p>
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<p>Convergence of CI calculations for transition rates in He-like Ni.</p>
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<p>Convergence of CI calculations for transition rates in Li-like Ni.</p>
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<p>FAC input written in Python language, used to generate atomic data for subsequent CRM simulations.</p>
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<p>Example of FAC input written in Python language, used to perform CRM simulations.</p>
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<p>Recreated experimental spectrum from Bombarda et al. [<a href="#B3-atoms-13-00018" class="html-bibr">3</a>] (dots) compared to spectra simulated by FAC (dashed and solid lines).</p>
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<p>FAC CRM simulations for the X-ray spectra originating from the Ni<sup>26+</sup>, Ni<sup>25+</sup>, Ni<sup>24+</sup>, and Ni<sup>23+</sup> ions in the 1.585–1.620 Å wavelength range and 2–8 keV electron temperature range.</p>
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<p>FAC CRM simulations for the X-ray spectra originating from the Ni<sup>26+</sup> ions in the 1.585–1.620 Å wavelength range and 2–8 keV electron temperature range.</p>
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<p>FAC CRM simulations for the X-ray spectra originating from the Ni<sup>25+</sup> ions in the 1.585–1.599 Å wavelength range and 2–8 keV electron temperature range.</p>
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<p>FAC CRM simulations for the X-ray spectra originating from the Ni<sup>24+</sup> ions in the 1.585–1.620 Å wavelength range and 2–8 keV electron temperature range.</p>
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<p>FAC CRM simulations for the X-ray spectra originating from the Ni<sup>23+</sup> ions in the 1.585–1.599 Å wavelength range and 2–8 keV electron temperature range.</p>
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<p>Approximation of the <math display="inline"><semantics> <mrow> <mi>n</mi> <mo>≥</mo> <mn>3</mn> </mrow> </semantics></math> satellites of Ni<sup>25+</sup> lying in the range 1.588–1.592 Å by using three Gaussians.</p>
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14 pages, 2030 KiB  
Article
Analysis of Dissipation Mechanisms for Cesium Rydberg Atoms in Magic-Wavelength Optical Trap
by Shaofeng Fan, Yang Liu, Wenyuan Liu, Yang Zhao, Yijun Li and Jiandong Bai
Photonics 2025, 12(2), 138; https://doi.org/10.3390/photonics12020138 - 8 Feb 2025
Viewed by 565
Abstract
A magic optical dipole trap (ODT) can confine atoms in the ground state and a highly excited state with the same light shifts, resulting in a long-range coherent lifetime between them, which plays an important role in high-fidelity quantum logic gates, multi-body physics [...] Read more.
A magic optical dipole trap (ODT) can confine atoms in the ground state and a highly excited state with the same light shifts, resulting in a long-range coherent lifetime between them, which plays an important role in high-fidelity quantum logic gates, multi-body physics and other quantum information. Here, we use a sum-over-states model to calculate the dynamic polarizabilities of the 6S1/2 ground state and 46S1/2 Rydberg state of Cs atoms and identify corresponding magic wavelengths and magic detunings for trapping the two states in the range of 900–1950 nm. Then, we analyze the robustness of the magic condition and the feasibility of the experimental operation. Furthermore, we estimate the trapping lifetime of Cs Rydberg atoms by considering different dissipation mechanisms, such as photon scattering and photoionization in the magic ODT. The photoexcitation and photoionization of Cs atoms under the action of three-step laser pulses are calculated by the rate equation. The presented results for magic-wavelength ODTs are of great significance for quantum information and quantum computing based on Rydberg atoms. Full article
(This article belongs to the Special Issue Optical Quantum System)
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<p>Magic ODT for ground state and Rydberg state of Cs atoms. (<b>a</b>) The traditional far-off-resonance red-detuned ODT has an attractive potential for ground-state atoms, but it shows a repulsive potential for Rydberg atoms. (<b>b</b>) For a magic-wavelength ODT, the ground state and Rydberg state have the same potential trap.</p>
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<p>(<b>a</b>) The dynamic polarizabilities of the 6S<sub>1/2</sub> ground state (black dotted line) and 46S<sub>1/2</sub> Rydberg state (red solid line) in the range of 900–1950 nm. (<b>b</b>) The dynamic polarizability near the 46S<sub>1/2</sub> ↔ 7P<sub>3/2</sub> auxiliary transition. When the detuning is +1.5897 GHz relative to the transition of 46S<sub>1/2</sub> ↔ 7P<sub>3/2</sub>, the ODT has an attractive potential for the ground state and Rydberg state.</p>
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<p>The relative potential well depth varies with the change in the ODT laser wavelength for trapping the 6S<sub>1/2</sub> ground state and 46S<sub>1/2</sub> Rydberg state.</p>
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<p>The laser power of different optical traps varies with the beam waist radius.</p>
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<p>Schematic diagram of three-step photoexcitation and photoionization of Cs atoms.</p>
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<p>Photoionization of Cs atom with the second- (<b>a</b>) and third-step (<b>b</b>) laser power.</p>
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<p>The variations in the population rates of the 6S<sub>1/2</sub> ground state—(<b>a</b>), 6P<sub>3/2</sub> excited state—(<b>b</b>), 46S<sub>1/2</sub> Rydberg state—(<b>c</b>), and the ionized state—(<b>d</b>) with laser pulse width.</p>
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17 pages, 476 KiB  
Article
Linking Planetary Ephemeris Reference Frames to ICRF via Millisecond Pulsars
by Li Guo, Yueqi Song, Zhen Yan, Liang Li and Guangli Wang
Universe 2025, 11(2), 54; https://doi.org/10.3390/universe11020054 - 7 Feb 2025
Viewed by 384
Abstract
The positions of millisecond pulsars (MSPs) can be determined with sub-milliarcsecond (mas) accuracy using both Very Long Baseline Interferometry (VLBI) and timing, referenced to the International Celestial Reference Frame (ICRF) and planetary ephemerides frame, respectively, representing kinematic and dynamical reference frames. The two [...] Read more.
The positions of millisecond pulsars (MSPs) can be determined with sub-milliarcsecond (mas) accuracy using both Very Long Baseline Interferometry (VLBI) and timing, referenced to the International Celestial Reference Frame (ICRF) and planetary ephemerides frame, respectively, representing kinematic and dynamical reference frames. The two frames can be connected through observations of common celestial objects, MSPs observed with VLBI and timing. However, previous attempts to establish this connection were unreliable due to the limited number of MSPs observed by both techniques. Currently, 23 MSPs have been precisely measured using both multiple timing and VLBI networks. Among them, 17 MSPs are used to link the two reference frames, marking a significant three-fold increase in the number of common MSPs used for frame linking. Nevertheless, six MSPs located near the ecliptic plane are excluded from frame linkage due to positional differences exceeding 20 mas measured by VLBI and timing. This discrepancy is primarily attributed to errors introduced in fitting positions in timing methods. With astrometric parameters obtained via both VLBI and timing for these MSPs, the precision of linking DE436 and ICRF3 has surpassed 0.4 mas. Furthermore, thanks to the improved timing precision of MeerKAT, even with data from just 13 MSPs observed by both MeerKAT and VLBI, the precision of linking DE440 and ICRF3 can also exceed 0.4 mas. The reliability of this linkage depends on the precision of pulsar astrometric parameters, their spatial distribution, and discrepancies in pulsar positions obtained by the two techniques. Notably, proper motion differences identified by the two techniques are the most critical factors influencing the reference frame linking parameters. The core shift of the calibrators in VLBI pulsar observations is one of the factors causing proper motion discrepancies, and multi-wavelength observations are expected to solve it. With the improvement in timing accuracy and the application of new observation modes like multi-view and multi-band observations in VLBI, the linkage accuracy of the dynamical and kinematic reference frames is expected to reach 0.3 mas. Full article
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<p>Spatial distribution of 23 MSPs measured via VLBI and timing in the equatorial coordinate system. The red star indicates MSPs from IPTA DR2, while blue circles represent MSPs from MPTA DR1.</p>
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<p>Position differences of pulsars between DE436 and ICRF3 at the epoch of MJD 55000.0.</p>
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10 pages, 2484 KiB  
Article
Switchable Negative Group Delay Based on Sandwich Topological Protection Structure in Terahertz Band
by Jiao Xu, Xianmin Pan, Jiao Tang, Xianghua Peng and Yuxiang Peng
Nanomaterials 2025, 15(4), 251; https://doi.org/10.3390/nano15040251 - 7 Feb 2025
Viewed by 430
Abstract
A switchable enhancement group delay in the terahertz band based on a novel sandwich topology protection structure with graphene is proposed in this paper. The notable phase transition of the reflected beam comes from the topological edge-protected mode excited at the sandwich photonic [...] Read more.
A switchable enhancement group delay in the terahertz band based on a novel sandwich topology protection structure with graphene is proposed in this paper. The notable phase transition of the reflected beam comes from the topological edge-protected mode excited at the sandwich photonic crystal surface, and the non-trivial topology of the photonic crystal allows the structure to be immune against defects and imperfections, which lays the foundation for the enhancement of group delay in the terahertz band. And the introduction of graphene creates favorable conditions for the reversible switching of positive and negative reflection group delay. Moreover, the reflected group delay can also be flexibly and dynamically controlled by the incident angle. The positive and negative reversible switching reflected group delay proposed in the terahertz band greatly reduces the optical transmission loss and significantly increases the transmission efficiency compared with the traditional metal sandwich structure, which provides a feasible idea for the realization of multi-dimensional manipulation of the wavelength and phase of electromagnetic waves in the terahertz band. The novel scheme is expected to provide potential applications in fields such as optical buffers or ultrafast modulators. Full article
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<p>Schematic diagram of a topological protection structure at THz frequencies. The incidence angle is θ.</p>
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<p>(<b>a</b>) The reflectance spectra of α-type (red, short-dashed line), β-type (cyan, short-dotted line), the “α+β” heterostructure (blue, solid line) and the “α+graphene+β” (pink, dash-dotted line); (<b>b</b>) Electric field distribution of topological sandwich structure; (<b>c</b>) The energy band of topological sandwich structure.</p>
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<p>Dependence of the (<b>a</b>) reflected phase, <math display="inline"><semantics> <mrow> <msub> <mrow> <mi mathvariant="sans-serif">ϕ</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math>, and (<b>b</b>) reflected group delay, <math display="inline"><semantics> <mrow> <msub> <mrow> <mi mathvariant="normal">τ</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math>, on frequency for different Fermi energies of graphene. For comparison, reflected phase and group delay without graphene is shown as well (red solid line).</p>
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<p>Dependence of the reflected group delay, <math display="inline"><semantics> <mrow> <msub> <mrow> <mi mathvariant="normal">τ</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math>, on frequency for different relaxation times, τ, of graphene.</p>
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<p>Dependence of the (<b>a</b>) reflected phase, <math display="inline"><semantics> <mrow> <msub> <mrow> <mi mathvariant="sans-serif">ϕ</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math>, and (<b>b</b>) reflected group delay, <math display="inline"><semantics> <mrow> <msub> <mrow> <mi mathvariant="normal">τ</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math>, on frequency for different incident angles with graphene (black line), without graphene (red line).</p>
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<p>Dependence of the (<b>a</b>) reflected phase, <math display="inline"><semantics> <mrow> <msub> <mrow> <mi mathvariant="sans-serif">ϕ</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math>, and (<b>b</b>,<b>c</b>) reflected group delay, <math display="inline"><semantics> <mrow> <msub> <mrow> <mi mathvariant="normal">τ</mi> </mrow> <mrow> <mi mathvariant="normal">r</mi> </mrow> </msub> </mrow> </semantics></math>, on frequency for different N layers of graphene.</p>
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12 pages, 1901 KiB  
Article
Advancing Near-Infrared Probes for Enhanced Breast Cancer Assessment
by Mohammad Pouriayevali, Ryley McWilliams, Avner Bachar, Parmveer Atwal, Ramani Ramaseshan and Farid Golnaraghi
Sensors 2025, 25(3), 983; https://doi.org/10.3390/s25030983 - 6 Feb 2025
Viewed by 409
Abstract
Breast cancer remains a leading cause of cancer-related deaths among women, emphasizing the critical need for early detection and monitoring techniques. Conventional imaging modalities such as mammography, MRI, and ultrasound have face sensitivity, specificity, cost, and patient comfort limitations. This study introduces a [...] Read more.
Breast cancer remains a leading cause of cancer-related deaths among women, emphasizing the critical need for early detection and monitoring techniques. Conventional imaging modalities such as mammography, MRI, and ultrasound have face sensitivity, specificity, cost, and patient comfort limitations. This study introduces a handheld Near-Infrared Diffuse Optical Tomography (NIR DOT) probe for breast cancer imaging. The NIRscan probe utilizes multi-wavelength light-emitting diodes (LEDs) and a linear charge-coupled device (CCD) sensor to acquire real-time optical data, reconstructing cross-sectional images of breast tissue based on scattering and absorption coefficients. With wavelengths optimized for the differential optical properties of tissue components, the probe enables functional imaging, distinguishing between healthy and malignant tissues. Clinical evaluations have demonstrated its potential for precise tumor localization and monitoring therapeutic responses, achieving a sensitivity of 94.7% and specificity of 84.2%. By incorporating machine learning algorithms and a modified diffusion equation (MDE), the system enhances the accuracy and speed of image reconstruction, supporting rapid, non-invasive diagnostics. This development represents a significant step forward in portable, cost-effective solutions for breast cancer detection, with potential applications in low-resource settings and diverse clinical environments. Full article
(This article belongs to the Special Issue Advanced Sensors for Detection of Cancer Biomarkers and Virus)
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<p>Face of probe head [<a href="#B1-sensors-25-00983" class="html-bibr">1</a>].</p>
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<p>System architecture of the NIR handheld probe, showing the integration of the ARM Cortex M4 microcontroller, ADC, CCD sensor, and light source control [<a href="#B1-sensors-25-00983" class="html-bibr">1</a>].</p>
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<p>The custom software’s graphical user interface (GUI) version 0.4 is presented on a Windows platform.</p>
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<p>An optical image of a physical phantom with a 4.5 mm spherical abnormality at the center was captured at 690 nm [<a href="#B1-sensors-25-00983" class="html-bibr">1</a>].</p>
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<p>Reconstructed 3D optical image of a patient’s tumor using 12 slices at 690 nm: (<b>a</b>) Reconstructed image using the NIR probe’s MDE imaging. (<b>b</b>) A 3D volume model of the tumor created using MATLAB rendering capabilities with gaps between the adjacent slices interpolated [<a href="#B19-sensors-25-00983" class="html-bibr">19</a>].</p>
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<p>Diagram illustrating the photon propagation paths in a highly scattering medium. LED light travels along multiple, semi-circular paths through the tissue, converging at various points [<a href="#B19-sensors-25-00983" class="html-bibr">19</a>].</p>
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22 pages, 18158 KiB  
Article
A Novel Model for Noninvasive Haemoglobin Detection Based on Visibility Network and Clustering Network for Multi-Wavelength PPG Signals
by Lei Liu, Ziyi Wang, Xiaohan Zhang, Yan Zhuang and Yongbo Liang
Algorithms 2025, 18(2), 75; https://doi.org/10.3390/a18020075 - 1 Feb 2025
Viewed by 445
Abstract
Non-invasive haemoglobin (Hb) testing devices enable large-scale haemoglobin screening, but their accuracy is not comparable to traditional blood tests. To this end, this paper aims to design a non-invasive haemoglobin testing device and propose a classification-regression prediction framework for non-invasive testing of haemoglobin [...] Read more.
Non-invasive haemoglobin (Hb) testing devices enable large-scale haemoglobin screening, but their accuracy is not comparable to traditional blood tests. To this end, this paper aims to design a non-invasive haemoglobin testing device and propose a classification-regression prediction framework for non-invasive testing of haemoglobin using visibility graphs (VG) with network clustering of multi-sample pulse-wave-weighted undirected graphs as the features to optimize the detection accuracy of non-invasive haemoglobin measurements. Different prediction methods were compared by analyzing 608 segments of multiwavelength fingertip PPG signal data from 152 volunteers and analyzing and comparing the data and methods. The results showed that the classification using NVG with complex network clustering as features in the interval classification model was the best, with its classification accuracy (acc) of 93.35% and model accuracy of 88.28%. Among the regression models, the classification regression stack: SVM-Light Gradient Boosting Machine (LGBM) was the most effective, with a Mean Absolute Error (MAE) of 6.67 g/L, a Root Mean Square Error (RMSE) of 8.21 g/L, and an R-Square (R2) of 0.64. The results of this study indicate that the use of complex network technology in non-invasive haemoglobin detection can effectively improve its accuracy, and the detector designed in this study is promising to carry out a more accurate large-scale haemoglobin screening. Full article
(This article belongs to the Special Issue Advanced Research on Machine Learning Algorithms in Bioinformatics)
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<p>The figure shows the general flow of the research. It mainly includes three main processes and nine subplots from developing signal acquisition equipment to acquiring data sets, then constructing a predictive model from the data sets, and developing the corresponding host computer to apply the model.</p>
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<p>The figure shows the exterior of the MW-PPG signal acquisition device and the internal structure of the sensor.</p>
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<p>A block diagram of the interface between the MW-PPG signal acquisition system and the Hb detection system is shown in the figure. Figure (<b>A</b>) shows the block diagram of the interface of the signal acquisition system and Figure (<b>B</b>) shows the block diagram of the interface of the detection system.</p>
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<p>This figure shows the basic information of the Hb dataset: (<b>A</b>) shows a histogram of the distribution of Hb intervals and gender and (<b>B</b>) shows a histogram of the distribution of Hb and age.</p>
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<p>This figure illustrates the flowchart for the extraction of viewable features in complex networks.</p>
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<p>(<b>A</b>) shows the data preprocessing process and (<b>B</b>) shows the PPG signal morphological features used in generating multi-sample complex networks, where A1 A2 is the area of the PPG signal cycle in the figure divided by the boundary line.</p>
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<p>This figure shows the schematic process of transforming MW-PPG signaling features into a multi-sample clustering network. Within the row vectors in the figure are the features in <a href="#algorithms-18-00075-t001" class="html-table">Table 1</a>.</p>
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<p>Schematic Diagram of the Stacked Classification and Regression Prediction Framework.</p>
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<p>Statistical Histogram of Clustering Results. (<b>A</b>) Clustering Distribution of four different types, with Cluster I noted as high Hb, Clusters II and III noted as normal Hb, and Cluster IV as low Hb. And Figure B demonstrates the histogram of the overlap between the clustering results and the hemoglobin distribution.</p>
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<p>Figure (<b>A</b>) illustrates the rules for generating natural visibility graphs and network heat maps, while Figure (<b>B</b>) shows the rules for generating horizontal visibility graphs and network heat maps.</p>
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<p>Figure (<b>A</b>) shows the accuracy of the proposed classification model, which worked as NVG-cluster, NVG, HVG-cluster, and HVG, four different feature inputs under different feature numbers. Figure (<b>B</b>) shows the confusion matrix for classification models using NVG and clustered features.</p>
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<p>These figures are individual model indicator box plots. Figure (<b>A</b>) shows a comparison for MAE, Figure (<b>B</b>) shows a comparison for R2, and Figure (<b>C</b>) shows a comparison for RMSE.</p>
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<p>The scatterplot of the results of the categorical regression confounding model using the new features as well as the Altman plot are presented in this figure.</p>
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<p>This figure illustrates the roadmap for future improvements in this study.</p>
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22 pages, 4847 KiB  
Article
Extracting the Spatial Correlation of Wall Pressure Fluctuations Using Physically Driven Artificial Neural Network
by Jian Sun, Xinyuan Chen, Yiqian Zhang, Jinan Lv and Xiaojian Zhao
Aerospace 2025, 12(2), 112; https://doi.org/10.3390/aerospace12020112 - 31 Jan 2025
Viewed by 484
Abstract
The spatial correlation of wall pressure fluctuations is a crucial parameter that affects the structural vibration caused by a turbulent boundary layer (TBL). Although the phase-array technique is commonly used in industry applications to obtain this correlation, it has proven to be effective [...] Read more.
The spatial correlation of wall pressure fluctuations is a crucial parameter that affects the structural vibration caused by a turbulent boundary layer (TBL). Although the phase-array technique is commonly used in industry applications to obtain this correlation, it has proven to be effective only for moderate frequencies. In this study, an artificial neural network (ANN) method was developed to calculate the convective speed, indicating the spatial correlation of wall pressure fluctuations and extending the frequency range of the conventional phase-array technique. The developed ANN system, based on a radial basis function (RBF), has been trained using discrete simulated data that follow the physical essence of wall pressure fluctuations. Moreover, a normalization method and a multi-parameter average (MPA) method have been employed to improve the training of the ANN system. The results of the investigation demonstrate that the MPA method can expand the frequency range of the ANN, enabling the maximum analysis frequency of convective velocity for aircraft wall pressure fluctuations to reach over 10 kHz. Furthermore, the results reveal that the ANN technique is not always effective and can only accurately calculate the wavenumber when the standard wavelength is less than four times the width of the sensor array along the flow direction. Full article
(This article belongs to the Section Aeronautics)
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<p>TBL wavenumber–frequency spectrum.</p>
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<p>RBF network diagram.</p>
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<p>Results of the leave-one-out cross validation: (<b>a</b>) <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>Ε</mi> </mrow> <mrow> <mi>m</mi> <mi>s</mi> <mi>e</mi> </mrow> </msub> <mo>=</mo> <msup> <mrow> <mn>10</mn> </mrow> <mrow> <mo>−</mo> <mn>1</mn> </mrow> </msup> </mrow> </semantics></math>, (<b>b</b>) <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>Ε</mi> </mrow> <mrow> <mi>m</mi> <mi>s</mi> <mi>e</mi> </mrow> </msub> <mo>=</mo> <msup> <mrow> <mn>10</mn> </mrow> <mrow> <mo>−</mo> <mn>2</mn> </mrow> </msup> </mrow> </semantics></math>, (<b>c</b>) <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>Ε</mi> </mrow> <mrow> <mi>m</mi> <mi>s</mi> <mi>e</mi> </mrow> </msub> <mo>=</mo> <msup> <mrow> <mn>10</mn> </mrow> <mrow> <mo>−</mo> <mn>3</mn> </mrow> </msup> </mrow> </semantics></math>, and (<b>d</b>) <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>Ε</mi> </mrow> <mrow> <mi>m</mi> <mi>s</mi> <mi>e</mi> </mrow> </msub> <mo>=</mo> <mn>0</mn> </mrow> </semantics></math>.</p>
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<p>Comparison between the ANN and the reference method: (<b>a</b>) <math display="inline"><semantics> <mrow> <mi>f</mi> <mo>=</mo> </mrow> </semantics></math>100 Hz and (<b>b</b>) <math display="inline"><semantics> <mrow> <mi>f</mi> <mo>=</mo> </mrow> </semantics></math>500 Hz.</p>
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<p>Identification results by ANN at low and high frequencies: (<b>a</b>) <math display="inline"><semantics> <mrow> <mi>f</mi> <mo>=</mo> </mrow> </semantics></math>10 Hz and (<b>b</b>) <math display="inline"><semantics> <mrow> <mi>f</mi> <mo>=</mo> </mrow> </semantics></math>10,000 Hz.</p>
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<p>Measurement model design and setup.</p>
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<p>Comparison between the ANN and the conventional method in the high-frequency range.</p>
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<p>Low-frequency effect on ANN identification.</p>
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<p>Comparison between the ANN and the conventional method across the entire frequency range.</p>
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<p>Identification results with different flow velocities.</p>
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<p>Identification results for different standard wavelengths.</p>
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<p>Wall pressure fluctuations for different standard wavelengths.</p>
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<p>Different sensor distribution selected from the original sensor array: (<b>a</b>) linear, (<b>b</b>) circular, (<b>c</b>) cross, and (<b>d</b>) sparse.</p>
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<p>The effect of the array form on convective speed calculation.</p>
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<p>Local measurement data map: (<b>a</b>) all the test points included, and (<b>b</b>) with invalid data removed.</p>
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<p>Impact of failed test points on convective speed calculation.</p>
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49 pages, 68388 KiB  
Article
Improved Stereophotogrammetric and Multi-View Shape-from-Shading DTMs of Occator Crater and Its Interior Cryovolcanism-Related Bright Spots
by Alicia Neesemann, Stephan van Gasselt, Ralf Jaumann, Julie C. Castillo-Rogez, Carol A. Raymond, Sebastian H. G. Walter and Frank Postberg
Remote Sens. 2025, 17(3), 437; https://doi.org/10.3390/rs17030437 - 27 Jan 2025
Viewed by 472
Abstract
Over the course of NASA’s Dawn Discovery mission, the onboard framing camera mapped Ceres across a wide wavelength spectrum at varying polar science orbits and altitudes. With increasing resolution, the uniqueness of the 92 km wide, young Occator crater became evident. Its central [...] Read more.
Over the course of NASA’s Dawn Discovery mission, the onboard framing camera mapped Ceres across a wide wavelength spectrum at varying polar science orbits and altitudes. With increasing resolution, the uniqueness of the 92 km wide, young Occator crater became evident. Its central cryovolcanic dome, Cerealia Tholus, and especially the associated bright carbonate and ammonium chloride deposits—named Cerealia Facula and the thinner, more dispersed Vinalia Faculae—are the surface expressions of a deep brine reservoir beneath Occator. Understandably, this made this crater the target for future sample return mission studies. The planning and preparation for this kind of mission require the characterization of potential landing sites based on the most accurate topography and orthorectified image data. In this work, we demonstrate the capabilities of the freely available and open-source USGS Integrated Software for Imagers and Spectrometers (ISIS 3) and Ames Stereo Pipeline (ASP 2.7) in creating high-quality image data products as well as stereophotogrammetric (SPG) and multi-view shape-from-shading (SfS) digital terrain models (DTMs) of the aforementioned spectroscopically challenging features. The main data products of our work are four new DTMs, including one SPG and one SfS DTM based on High-Altitude Mapping Orbit (HAMO) (CSH/CXJ) and one SPG and one SfS DTM based on Low-Altitude Mapping Orbit (LAMO) (CSL/CXL), along with selected Extended Mission Orbit 7 (XMO7) framing camera (FC) data. The SPG and SfS DTMs were calculated to a GSD of 1 and 0.5 px, corresponding to 136 m (HAMO SPG), 68 m (HAMO SfS), 34 m (LAMO SPG), and 17 m (LAMO SfS). Finally, we show that the SPG and SfS approaches we used yield consistent results even in the presence of high albedo differences and highlight how our new DTMs differ from those previously created and published by the German Aerospace Center (DLR) and the Jet Propulsion Laboratory (JPL). Full article
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<p>CSH CYCLE 1 photometrically corrected RGB orthomosaic of the Occator crater (F5IR, F2GREEN, F8BLUE). The map is a stereographic projection with the projection and image center at 22.879°N<sub><math display="inline"><semantics> <mi>φ</mi> </semantics></math></sub>/239.429°E (19.865°N<sub><math display="inline"><semantics> <mi>ψ</mi> </semantics></math></sub>). RGB values were limited to R: 0.0257–0.0339; G: 0.0555–0.0869; and B: 0.0552–0.0815. (<b>a</b>) Due to the high albedo difference, bright deposits within Occator appear overexposed in the applied histogram stretch. To get an idea about their shape and distribution, we compiled a CSL/CXL RGB orthomosaic with a histogram stretch optimized for the bright deposits, shown in <a href="#remotesensing-17-00437-f002" class="html-fig">Figure 2</a>. (<b>b</b>) Extent of our CSL/CXL ASP SPG DTM. (<b>c</b>,<b>d</b>) Areas for which we calculated the highest resolution DTM (CSL/CXL ASP SfS DTMs).</p>
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<p>Photometrically corrected CSL/CXL RGB orthomosaic of Occator’s interior. The mosaic was compiled from 13 individual images per channel (see <a href="#remotesensing-17-00437-t0A2" class="html-table">Table A2</a>) using F5IR, F2GREEN, and F8BLUE as the three RGB bands. In contrast to <a href="#remotesensing-17-00437-f001" class="html-fig">Figure 1</a>, images were photometrically corrected based on the 482 × 446 km ellipsoid, not on the DTM, to preserve the topography-related brightness variations and morphology, respectively. RGB values were limited to R: 0.0016–0.6634; G: 0.0003–1.5579; and B: 0.0000–1.1953. The figure is a stereographic projection centered at 23.05°N<sub><math display="inline"><semantics> <mi>φ</mi> </semantics></math></sub>/241.05°E (20.02°N<sub><math display="inline"><semantics> <mi>ψ</mi> </semantics></math></sub>). To the left, we see Cerealia Facula with its fractured dome, Cerealia Tholus, and the orange-colored exposed hydrated sodium chloride [<a href="#B24-remotesensing-17-00437" class="html-bibr">24</a>]. To the right, we see various smaller and thinner bright deposits collectively named Vinalia Faculae (<b>a</b>–<b>e</b>).</p>
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<p>Number of acquired FC2 images and geometries of polar mapping orbits during Dawn’s mission at Ceres. Left: Number of images acquired by the FC2 during Dawn’s mission to Ceres. Left: During the course of Dawn’s mission at Ceres, 67,969 images in total were acquired by the FC2. Except for images acquired for the purpose of the camera calibration and orientation of the spacecraft, as well as for the search of moons orbiting Ceres, by far the most images mapping Ceres directly were taken during the HAMO and LAMO. Ancillary image acquisition was carried out by the FC1 in order to increase spatial coverage during Dawn’s time-limited final mission phase, XM2, but is not included in this figure (see <a href="#remotesensing-17-00437-t001" class="html-table">Table 1</a>). Right: Indicated orbits correspond to the median distance to Ceres’ center during the different orbit phases. 360° corresponds to the period between 2015/01/01 and 2018/12/31. Geometries of Dawn’s highly elliptical 2nd extended mission orbits (XMO5–XMO7) flown during the final mission, extended mission XM2, are not shown in this figure for scale reasons.</p>
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<p>Detection of erroneous pixels. In the upper two rows, we present average images created for the eight individual FC filters and two average flat-field images for the F1 and F7 filters taken while the front door was closed and the calibration lamp (callamp) on. Note that images used in this context were not photometrically but only radiometrically corrected. The east–west shading therefore stems from the illumination conditions during image acquisition and not from camera shading. The five static erroneous pixel clusters recognized in all the average images are marked by an ‘x’ in the upper left subfigure. In the bottom row, we present magnifications of the five erroneous pixel clusters to illustrate their extent, marked by the dashed outlines. A 3 sigma histogram stretch was applied to each average image.</p>
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<p>Basic ISIS 3 pre-processing workflow. Gray: functions; red: temporary textfiles (here, GCP.net files); green: temporary raster files; blue: final photometrically corrected, orthorectified F1CLEAR image; yellow: F1CLEAR orthomosaic, HAMO-based SPG DTM, and reconstructed SPICE kernels. The asterisk in campt* stands for a script we wrote that reads out the lat/lon values at a specific sample/line position, converts them into cartesian coordinates (the ApprioryX, Y, and Z values) and creates a <span class="html-italic">qtie</span>-readable GCP netfile. A detailed description of the flowchart is given in <a href="#sec4dot4-remotesensing-17-00437" class="html-sec">Section 4.4</a>.</p>
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<p>ASP SPG processing workflow. This figure is a version of Figure 14.1 from the ASP 2.7 documentation (<a href="https://stereopipeline.readthedocs.io/en/latest/correlation.html" target="_blank">https://stereopipeline.readthedocs.io/en/latest/correlation.html</a>, accessed on 23 Decemeber 2024) that we have modified. The parameters specified in the stereo.txt file and passed to the <span class="html-italic">stereo</span> command are listed in Appendix <a href="#remotesensing-17-00437-t0A8" class="html-table">Table A8</a>. Other parameters passed to the <span class="html-italic">point2dem</span> command to remove additional erroneous points from the point cloud during the DTM generation are described in <a href="#sec4dot5-remotesensing-17-00437" class="html-sec">Section 4.5</a>.</p>
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<p>Latitude- and longitude-dependent deviation between the CSH/CXJ and CSL/CXL ASP SPG and SfS DTMs created in our study. For the upper two plots, the mean latitude and longitude values were calculated from the extent of area 1, while they were calculated for area 4 in the four lower plots.</p>
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<p>Latitude- and longitude-dependent deviation between the HAMO and LAMO SPG DTMs. Mean latitude and longitude values were calculated for the extent of area 3.</p>
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<p>Latitude- and longitude-dependent deviation of our 4 new CSH/CXJ and CSL/CXL SPG and SfS DTMs and the JPL HAMO/LAMO SPC DTM [<a href="#B58-remotesensing-17-00437" class="html-bibr">58</a>,<a href="#B59-remotesensing-17-00437" class="html-bibr">59</a>] from the DLR HAMO SPG DTM [<a href="#B55-remotesensing-17-00437" class="html-bibr">55</a>,<a href="#B56-remotesensing-17-00437" class="html-bibr">56</a>].</p>
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<p>Visual comparison of the seven DTMs for the example of the fresh crater located at 14.281°N<sub><math display="inline"><semantics> <mi>φ</mi> </semantics></math></sub>/233.489°E (12.295°N<sub><math display="inline"><semantics> <mi>ψ</mi> </semantics></math></sub>). Images used to create the orthomosaics are listed in <a href="#remotesensing-17-00437-t0A5" class="html-table">Table A5</a>.</p>
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<p>Topographic profiles of the fresh crater. Subfigures (<b>a</b>,<b>b</b>) (left and middle panel) are stereographic projections centered at 14.281°N<sub><math display="inline"><semantics> <mi>φ</mi> </semantics></math></sub>/233.489°E (12.295°N<sub><math display="inline"><semantics> <mi>ψ</mi> </semantics></math></sub>). (<b>a</b>) Photometrically corrected FC2 F1CLEAR close-up view of the fresh crater. (<b>b</b>) Photometrically corrected RGB (F5IR, F2GREEN, F8BLUE) orthomosaic of the fresh crater. In total, we derived 52 profiles at 3 degree intervals between 24–90°, 144–177°, and 240–288° for each of the seven DTMs extending from the crater center. (<b>c</b>) (right panel) Average topographic profiles for each of the seven DTMs. <sup>a</sup> [<a href="#B59-remotesensing-17-00437" class="html-bibr">59</a>], <sup>b</sup> [<a href="#B58-remotesensing-17-00437" class="html-bibr">58</a>], <sup>c</sup> [<a href="#B106-remotesensing-17-00437" class="html-bibr">106</a>], <sup>d</sup> [<a href="#B104-remotesensing-17-00437" class="html-bibr">104</a>], <sup>e</sup> [<a href="#B56-remotesensing-17-00437" class="html-bibr">56</a>], <sup>f</sup> [<a href="#B55-remotesensing-17-00437" class="html-bibr">55</a>].</p>
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<p>Detailed comparison of the topographic profiles of the fresh crater. As a reference (black solid line), we used our new CSL/CXL ASP SfS DTM, as it has the highest effective resolution and the highest d/D ratio of 0.255 and plotted it together with the profiles extracted from the other six DTMs (<b>a</b>–<b>f</b>). Black and gray triangles mark the inflection points (the highest elevation of the rim crest) of our reference profile and the other profiles. Note that the highest congruence exists between profiles taken from our CSL/CXL ASP SfS, our CSL/CXL ASP SPG, and the DLR CSL/CXL SPG DTMs.</p>
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<p>Visual comparison of the seven DTMs for the example of the Cerealia Tholus at 22.626°N<sub><math display="inline"><semantics> <mi>φ</mi> </semantics></math></sub>/239.581°E (19.648°N<sub><math display="inline"><semantics> <mi>ψ</mi> </semantics></math></sub>). Images used to create the orthomosaics are listed in <a href="#remotesensing-17-00437-t0A6" class="html-table">Table A6</a>.</p>
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<p>Overview of the location of the topographic profile across the Cerealia Tholus. We created three different maps, each with their advantages and disadvantages, in order to show which specific surface features are covered by our topographic profile. Our 25,498 m long profile goes from west to east while crossing the highest elevations (the Lohri, Cerealia, and Kekri Tholus) within Occator. (<b>a</b>) Semi-transparent, color-coded CSL/CXL/XMO7 ASP SfS DTM overlaid on the corresponding hillshade model. Topography contour lines are plotted in 100 m intervals. (<b>b</b>) CSL/CXL RGB color composite of Cerealia Facula. (<b>c</b>) Generated slope map overlaid on a curvature map. This combined map highlights aspects of the surface’s shape or features, such as the circular and other rather subparallel fault systems as well as numerous little mounds, at a detailed level.</p>
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<p>Topographic profiles across the Cerealia Tholus.</p>
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<p>Topographic profiles across Vinalia Faculae. (<b>a</b>) Topographic profiles across Vinalia Faculae, extracted from our CSL/CXL SPG (black line) and SfS (dark grey line) DTMs, as well as the HAMO/LAMO-based SPC DTM (blue line) from the JPL. Additionally, the albedo along the profile line was extracted based on the photometrically corrected CSL/CXL F1CLEAR orthomosaic included in this study. (<b>b</b>) Deviations between the lower resolution yet more robust CSL/CXL ASP SPG DTM, the CSL/CXL ASP SfS DTM, and the HAMO/LAMO-based SPC DTM from the JPL. (<b>c</b>) The CSL/CXL ASP SfS DTM of Vinalia Faculae, represented as elevations above the 482 × 446 km ellipsoid. (<b>d</b>) Photometrically corrected CSL/CXL F1CLEAR orthomosaic of Vinalia Faculae. Both maps are stereographic projections, centered at 23.292°N<sub><math display="inline"><semantics> <mi>φ</mi> </semantics></math></sub>/242.487°E (20.234°N<sub><math display="inline"><semantics> <mi>ψ</mi> </semantics></math></sub>). The course of the topographic profiles shown in panel (<b>a</b>) is indicated by a black-and-green dashed line.</p>
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16 pages, 421 KiB  
Article
The Gaussian-Drude Lens: A Dusty Plasma Model Applicable to Observations Across the Electromagnetic Spectrum
by Adam Rogers
Universe 2025, 11(2), 40; https://doi.org/10.3390/universe11020040 - 26 Jan 2025
Viewed by 494
Abstract
When radiation from a background source passes through a cloud of cold plasma, diverging lensing occurs if the source and observer are well-aligned. Unlike gravitational lensing, plasma lensing is dispersive, increasing in strength with wavelength. The Drude model is a generalization of cold [...] Read more.
When radiation from a background source passes through a cloud of cold plasma, diverging lensing occurs if the source and observer are well-aligned. Unlike gravitational lensing, plasma lensing is dispersive, increasing in strength with wavelength. The Drude model is a generalization of cold plasma, including absorbing dielectric dust described by a complex index of refraction. The Drude lens is only dispersive for wavelengths shorter than the dust characteristic scale (λλd). At sufficient photon energy, the dust particles act like refractive clouds. For longer wavelengths λλd, the optical properties of the Drude lens are constant, unique behavior compared to the predictions of the cold plasma lens. Thus, cold plasma lenses can be distinguished from Drude lenses using multi-band observations. The Drude medium extends the applicability of all previous tools, from gravitational and plasma lensing, to describe scattering phenomena in the X-ray regime. Full article
(This article belongs to the Special Issue Recent Advances in Gravitational Lensing and Galactic Dynamics)
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Figure 1

Figure 1
<p>(<b>Left</b>): The Drude effective wavelength <math display="inline"><semantics> <mrow> <msubsup> <mi mathvariant="normal">Λ</mi> <mi>D</mi> <mn>2</mn> </msubsup> <mrow> <mo>(</mo> <mi>λ</mi> <mo>)</mo> </mrow> </mrow> </semantics></math> is plotted as a function of wavelength for four separate instances of the dust characteristic wavelength. The heavy curves represent the Rayleigh regime. The diagonal dashed line is the cold plasma case with <math display="inline"><semantics> <mrow> <msubsup> <mi mathvariant="normal">Λ</mi> <mi>D</mi> <mn>2</mn> </msubsup> <mo>=</mo> <msup> <mi>λ</mi> <mn>2</mn> </msup> </mrow> </semantics></math>. (<b>Right</b>): The Drude absorption coefficient <math display="inline"><semantics> <mrow> <msubsup> <mi mathvariant="normal">Λ</mi> <mi>D</mi> <mn>2</mn> </msubsup> <mo>/</mo> <msub> <mi>λ</mi> <mi>d</mi> </msub> </mrow> </semantics></math> is plotted as a function of wavelength for the dust characteristic wavelength cases given in the left panel. The diagonal dashed line is <math display="inline"><semantics> <mrow> <msubsup> <mi mathvariant="normal">Λ</mi> <mi>D</mi> <mn>2</mn> </msubsup> <mo>=</mo> <msup> <mi>λ</mi> <mn>2</mn> </msup> </mrow> </semantics></math>. Both plots are on log-log scales.</p>
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<p>An example of scattering. The source is seen through a scattering screen, which produces a scatter-broadened image. The apparent dimensions of the source are symmetrically stretched by a factor of <math display="inline"><semantics> <mrow> <mo>(</mo> <mn>1</mn> <mo>+</mo> <msub> <mi>θ</mi> <mi>S</mi> </msub> <mo>)</mo> </mrow> </semantics></math>.</p>
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<p>Imaging examples for (<b>Left</b>), the usual lensing geometry in the case of a refractive screen, and (<b>Right</b>), including both refraction and scattering. Similar to <a href="#universe-11-00040-f002" class="html-fig">Figure 2</a>, scattering broadens the apparent dimensions of the source.</p>
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Article
Graphene Quantum Dots in Bacterial Cellulose Hydrogels for Visible Light-Activated Antibiofilm and Angiogenesis in Infection Management
by Danica Z. Zmejkoski, Nemanja M. Zdravković, Dijana D. Mitić, Zoran M. Marković, Milica D. Budimir Filimonović, Dušan D. Milivojević and Biljana M. Todorović Marković
Int. J. Mol. Sci. 2025, 26(3), 1053; https://doi.org/10.3390/ijms26031053 - 26 Jan 2025
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Abstract
A novel bacterial cellulose (BC)-based composite hydrogel with graphene quantum dots (BC-GQDs) was developed for photodynamic therapy using blue and green light (BC-GQD_blue and BC-GQD_green) to target pathogenic bacterial biofilms. This approach aims to address complications in treating nosocomial infections and combating multi-drug-resistant [...] Read more.
A novel bacterial cellulose (BC)-based composite hydrogel with graphene quantum dots (BC-GQDs) was developed for photodynamic therapy using blue and green light (BC-GQD_blue and BC-GQD_green) to target pathogenic bacterial biofilms. This approach aims to address complications in treating nosocomial infections and combating multi-drug-resistant organisms. Short-term illumination (30 min) of both BC-GQD samples led to singlet oxygen production and a reduction in pathogenic biofilms. Significant antibiofilm activity (>50% reduction) was achieved against Staphylococcus aureus and Escherichia coli with BC-GQD_green, and against Pseudomonas aeruginosa with BC-GQD_blue. Atomic force microscopy images revealed a substantial decrease in biofilm mass, accompanied by changes in surface roughness and area, further confirming the antibiofilm efficacy of BC-GQDs under blue and green light, without any observed chemical alterations. Additionally, the biocompatibility of BC-GQDs was demonstrated with human gingival fibroblasts (HGFs). For the first time, in vitro studies explored the visible light-induced potential of BC-GQD composites to promote wound healing processes, showing increased migratory potential and the upregulation of eNOS and MMP9 gene expressions in HGFs. Chemical characterization revealed a 70 nm upshift in the photoluminescence emission spectra compared to the excitation wavelength. These novel photoactive BC-GQD hydrogel composites show great promise as effective agents for wound healing regeneration and infection management. Full article
(This article belongs to the Section Materials Science)
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<p>(<b>a</b>) Optical photographs of BC (<b>left</b>) and BC-GQD (<b>right</b>) samples; top-view AFM images of (<b>b</b>) BC-GQD_control (ambient light illumination), (<b>c</b>) BC-GQD_blue (blue light illumination at 470 nm), and (<b>d</b>) BC-GQD_green (green light illumination at 537 nm).</p>
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<p>FTIR spectra of BC-GQD_control (ambient light illumination; black curve), BC-GQD_blue (blue light illumination at 470 nm; blue curve), and BC-GQD_green (green light illumination at 537 nm; green curve).</p>
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<p>(<b>a</b>) PL intensity of BC-GQD hydrogel composites irradiated with blue light at 470 nm; (<b>b</b>) PL intensity of BC-GQD hydrogel composites irradiated with green light at 537 nm.</p>
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<p>EPR spectra of BC-GQD composite hydrogel samples illuminated with blue and green light (at 470 nm and 537 nm, respectively).</p>
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<p>Top-view AFM images of (<b>a</b>) well-formed <span class="html-italic">Pseudomonas aeruginosa</span> biofilm, (<b>b</b>) treated with BC-GQD_blue hydrogel composites and (<b>c</b>) treated with BC-QGD_green. The scanned surface for each image is 15 × 15 µm<sup>2</sup>.</p>
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<p>CLSM images of <span class="html-italic">Pseudomonas aeruginosa</span>’s biofilm before and after the treatment with the BC-GQD_green and BC-GQD_blue hydrogel composites. The scale bars are 20 µm.</p>
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<p>Biocompatibility tests—MTT and NRU. Mitochondrial activity and the proliferation of the cells seeded directly on the composites under ambient, blue, and green light illumination (BC-GQD_control, BC-GQD_blue, and BC-GQD_green, respectively) as well as with blue or green light alone. The values of the error bars are standard deviations; Kruskal–Wallis test was used, <span class="html-italic">p</span> &lt; 0.05.</p>
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<p>HGF migration induced via the application of BC-GQD_control, BC-GQD_blue, and BC-GQD_green at the following time intervals: start point and after 24 h (top and bottom row, respectively). Scale bar is 700 μm; Kruskal–Wallis test was used, * <span class="html-italic">p</span> &lt; 0.05.</p>
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<p><span class="html-italic">eNOS</span>, <span class="html-italic">MMP9</span>, and <span class="html-italic">Vimentin</span> relative gene expression after 72 h of HGF in the presence of the BC-GQD_control, BC-GQD_blue and BC-GQD_green composites, as well as blue and green light alone; Kruskal–Wallis test was used (* <span class="html-italic">p</span> &lt; 0.05, ** <span class="html-italic">p</span> &lt; 0.01, *** <span class="html-italic">p</span> &lt; 0.001, and **** <span class="html-italic">p</span> &lt; 0.0001). The values of the error bars are standard deviations.</p>
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