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11 pages, 5257 KiB  
Article
Simple Manufacturing of Large Polypyrrole Free-Standing Films Made of Nanoplatelets
by Cesar A. Barbero, Petr Slobodian, Robert Olejnik and Jiri Matyas
Nanomanufacturing 2025, 5(1), 4; https://doi.org/10.3390/nanomanufacturing5010004 - 7 Mar 2025
Viewed by 133
Abstract
A simple method is developed to produce free-standing films of polypyrrole (PPy) in one step. It consists of the interfacial polymerization (without surfactants) of pyrrole (dissolved in chloroform) with an oxidant (ammonium persulfate, dissolved in water). It is observed that the area of [...] Read more.
A simple method is developed to produce free-standing films of polypyrrole (PPy) in one step. It consists of the interfacial polymerization (without surfactants) of pyrrole (dissolved in chloroform) with an oxidant (ammonium persulfate, dissolved in water). It is observed that the area of the formed film only depends on the size of the interface, achieving the manufacture of PPy films of up to 300 cm2, with a thickness of 200 microns. Transmission electron microscopy (TEM) images show the presence of superimposed nanoplatelets of ca. 100 nm main axis. These nanoparticles seem to aggregate in two dimensions to form the free-standing film. Scanning electron microscopy (SEM) shows a compact surface with nanowires decorating the surface. PPy films show an electrical conductivity of 63 (±3) S cm−1. PPy conductive films are then applied in the construction of an antenna that shows a response in two bands: at 1.52 GHz (−13.85 dB) and at 3.50 GHz (−33.55 dB). The values are comparable to those of other antennas built with different PPy films. The simple synthesis of large-area PPy films in a single step would allow the fabrication of large quantities of electronic elements (e.g., sensors) with uniform properties in a short time. Full article
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Figure 1

Figure 1
<p>Photograph of the two-phase polymerization set-up, at an advanced state of film formation.</p>
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<p>Photograps of FEPPyF of increasing sizes.</p>
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<p>Photograph of large free-standing film of polypyrrole (fsPPyf).</p>
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<p>Scanning electron microscopy image of a typical fsPPy film surface.</p>
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<p>Transmission electron microscopy (TEM) of fsPPyF fragment.</p>
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<p>Plot of conductivity values obtained from table 3 of ref. [<a href="#B36-nanomanufacturing-05-00004" class="html-bibr">36</a>]. The red circle shows the conductivity of the free-standing films formed in this work.</p>
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<p>Photograph of the antenna containing a free-standing polypyrrole film.</p>
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<p>Measured return loss of the PPy antenna.</p>
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<p>Schematic of set-up of antenna made of polypyrrole (PPy) microstrip, ground plane, and coaxial cable.</p>
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<p>Mechanism of pyrrole polymerization and nanostructure formation.</p>
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26 pages, 34185 KiB  
Article
Design and Implementation of ESP32-Based Edge Computing for Object Detection
by Yeong-Hwa Chang, Feng-Chou Wu and Hung-Wei Lin
Sensors 2025, 25(6), 1656; https://doi.org/10.3390/s25061656 - 7 Mar 2025
Viewed by 179
Abstract
This paper explores the application of the ESP32 microcontroller in edge computing, focusing on the design and implementation of an edge server system to evaluate performance improvements achieved by integrating edge and cloud computing. Responding to the growing need to reduce cloud burdens [...] Read more.
This paper explores the application of the ESP32 microcontroller in edge computing, focusing on the design and implementation of an edge server system to evaluate performance improvements achieved by integrating edge and cloud computing. Responding to the growing need to reduce cloud burdens and latency, this research develops an edge server, detailing the ESP32 hardware architecture, software environment, communication protocols, and server framework. A complementary cloud server software framework is also designed to support edge processing. A deep learning model for object recognition is selected, trained, and deployed on the edge server. Performance evaluation metrics, classification time, MQTT (Message Queuing Telemetry Transport) transmission time, and data from various MQTT brokers are used to assess system performance, with particular attention to the impact of image size adjustments. Experimental results demonstrate that the edge server significantly reduces bandwidth usage and latency, effectively alleviating the load on the cloud server. This study discusses the system’s strengths and limitations, interprets experimental findings, and suggests potential improvements and future applications. By integrating AI and IoT, the edge server design and object recognition system demonstrates the benefits of localized edge processing in enhancing efficiency and reducing cloud dependency. Full article
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Figure 1
<p>Installation process of ESP32-CAM in Arduino IDE.</p>
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<p>ESP32-CAM module: 1.8-inch LCD (<b>left</b>), onboard camera (<b>right</b>).</p>
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<p>MQTT communication in the edge–cloud environment.</p>
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<p>Overall software framework.</p>
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<p>The software framework for the ESP32-CAM edge device.</p>
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<p>Cloud server software framework.</p>
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<p>Entire process from data collection to model deployment.</p>
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<p>The experimental setup for the image capture and recognition.</p>
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<p>Samples of testing images.</p>
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<p>Complete object detection process in the edge–cloud system.</p>
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<p>Response time of the Mosquitto broker (Option 1).</p>
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<p>Response time of the Mosquitto broker (Option 2).</p>
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<p>Response time of the Mosquitto broker (Option 3).</p>
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<p>Response time of the MQTTGO broker (Option 1).</p>
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<p>Response time of the MQTTGO broker (Option 2).</p>
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<p>Response time of the MQTTGO broker (Option 3).</p>
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<p>Response of the Eclipse broker (Option 1).</p>
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<p>Response time of the Eclipse broker (Option 2).</p>
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<p>Response time of the Eclipse broker (Option 3).</p>
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<p>Samples of validation images: person (<b>a</b>,<b>b</b>,<b>d</b>,<b>f</b>,<b>g</b>,<b>k</b>,<b>l</b>,<b>m</b>,<b>n</b>), non-person (<b>c</b>,<b>e</b>,<b>h</b>,<b>i</b>,<b>j</b>,<b>o</b>,<b>p</b>,<b>q</b>,<b>r</b>,<b>s</b>,<b>t</b>).</p>
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<p>Snap shots of object recognition under domestic broker and Option 3: (<b>a</b>) a person is detected, (<b>b</b>) object recognition by the edge, (<b>c</b>) object recognition by the cloud.</p>
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14 pages, 6225 KiB  
Article
Development of a Brain Catheter for Optical Coherence Tomography in Advanced Cerebrovascular Diagnostics
by Tae-Mi Jung, Tahsin Nairuz, Chang-Hyun Kim and Jong-Ha Lee
Biosensors 2025, 15(3), 170; https://doi.org/10.3390/bios15030170 - 6 Mar 2025
Viewed by 185
Abstract
Optical coherence tomography (OCT) has been extensively utilized in cardiovascular diagnostics due to its high resolution, rapid imaging capabilities; however, its adaptation for cerebrovascular applications remains constrained by the narrow, tortuous anatomical structure of cerebral vessels. To address these limitations, this study introduces [...] Read more.
Optical coherence tomography (OCT) has been extensively utilized in cardiovascular diagnostics due to its high resolution, rapid imaging capabilities; however, its adaptation for cerebrovascular applications remains constrained by the narrow, tortuous anatomical structure of cerebral vessels. To address these limitations, this study introduces a cerebrovascular-specific OCT (bOCT) catheter, an advanced adaptation of the cardiovascular OCT (cOCT) catheter, with significant structural modifications for improved access to brain blood vessels. The bOCT catheter incorporates a braided wire within a braided tube, strategically reinforcing axial strength. The distal shaft was reconfigured as a single-lumen structure, facilitating unified movement of the rotating fiber optic core and guidewire, thereby reducing guidewire bending and augmenting force transmission stability. Additionally, the anterior protrusion was removed and replaced with a dual-lumen configuration, significantly enhancing lesion accessibility. The bOCT catheter’s performance was validated in a 3D physical model and an animal model, demonstrating pronounced enhancements in flexibility, pushability, and navigability. Notably, the pushability through curved flow paths significantly improved, enhancing access to cerebral blood vessels. Therefore, this innovation promises to revolutionize cerebrovascular diagnostics with high-resolution imaging suited to the complex brain vasculature, setting a new standard in intravascular imaging technology. Full article
(This article belongs to the Section Optical and Photonic Biosensors)
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Figure 1
<p>Prototype bOCT catheter. (<b>A</b>) Whole catheter; (1) PIU (connector), (2) side-arm luer, (3) manifold, (4) proximal shaft (braided tube), (5) distal shaft (braided tube), (6) tip, (7) guidewire port/purge exit. (<b>B</b>) Guidewire through the proximal exit port on the side. (<b>C</b>) Guidewire through the entry port at the distal end.</p>
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<p>Schematic diagram of the segment of the bOCT catheter including the outer diameter (OD) and the inner diameter (ID). (<b>a</b>) Proximal braided shaft part (135 mm). (<b>b</b>) Proximal braided part (1130 mm). (<b>c</b>) Distal braided shaft part (270 mm). (<b>d</b>) Distal non-braided OCT lens part (30 mm).</p>
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<p>Surface contact angle after hydrophilic coating.</p>
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<p>Graph showing the trackability and pushability performance in the vascular simulated flow path according to the catheter specifications.</p>
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<p>Simulated blood vessel flow path (ASTM F2394) for investigating the mechanical performance of the cOCT and bOCT catheters. Distilled water was placed in the flow path instead of blood, and a 0.014-inch guidewire was used to analyze mechanical performance. The travel distance was set to 240 mm from the inlet to sufficiently observe catheter kinking. Kinking occurred at the enlarged flow point in the photo, and the maximum drag force at this point was measured.</p>
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<p>Insertion of the cOCT into the right external carotid artery. The catheter moves upward as it passes through a tortuous site.</p>
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<p>Insertion of the cOCT catheter into the right external carotid artery. The catheter no longer enters when tortuosity is exceeded.</p>
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<p>Insertion of the bOCT catheter into the right external carotid artery: good entry without excessive tension when passing through two areas of tortuosity.</p>
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30 pages, 14392 KiB  
Article
High-Quality Perovskite Thin Films for NO2 Detection: Optimizing Pulsed Laser Deposition of Pure and Sr-Doped LaMO3 (M = Co, Fe)
by Lukasz Cieniek, Agnieszka Kopia, Kazimierz Kowalski and Tomasz Moskalewicz
Materials 2025, 18(5), 1175; https://doi.org/10.3390/ma18051175 - 6 Mar 2025
Viewed by 108
Abstract
This study investigates the structural and catalytic properties of pure and Sr-doped LaCoO3 and LaFeO3 thin films for potential use as resistive gas sensors. Thin films were deposited via pulsed laser deposition (PLD) and characterized using X-ray diffraction (XRD), X-ray photoelectron [...] Read more.
This study investigates the structural and catalytic properties of pure and Sr-doped LaCoO3 and LaFeO3 thin films for potential use as resistive gas sensors. Thin films were deposited via pulsed laser deposition (PLD) and characterized using X-ray diffraction (XRD), X-ray photoelectron spectroscopy (XPS), scanning electron microscopy (SEM), atomic force microscopy (AFM), nanoindentation, and scratch tests. XRD analysis confirmed the formation of the desired perovskite phases without secondary phases. XPS revealed the presence of La3+, Co3+/Co4+, Fe3+/Fe4+, and Sr2+ oxidation states. SEM and AFM imaging showed compact, nanostructured surfaces with varying morphologies (shape and size of surface irregularities) depending on the composition. Sr doping led to surface refinement and increased nanohardness and adhesion. Transmission electron microscopy (TEM) analysis confirmed the columnar growth of nanocrystalline films. Sr-doped LaCoO3 demonstrated enhanced sensitivity and stability in the presence of NO2 gas compared to pure LaCoO3, as evidenced by electrical resistivity measurements within 230 ÷ 440 °C. At the same time, it was found that Sr doping stabilizes the catalytic activity of LaFeO3 (in the range of 300 ÷ 350 °C), although its behavior in the presence of NO2 differs from that of LaCo(Sr)O3—especially in terms of response and recovery times. These findings highlight the potential of Sr-doped LaCoO3 and LaFeO3 thin films for NO2 sensing applications. Full article
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Figure 1
<p>A representative example of the ABX<sub>3</sub> perovskite structure (<b>a</b>), along with its characteristic symmetry (<b>b</b>). The structural transformation scheme for LaMO<sub>3</sub> (M = Co, Fe) as a function of temperature is illustrated in (<b>c</b>). This transformation often leads to the formation of twin domains within the material, as depicted in (<b>d</b>).</p>
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<p>SEM images illustrating the surface topography of the targets used in the study; (<b>a</b>) LaCoO<sub>3</sub>, (<b>b</b>) La(Sr)CoO<sub>3</sub>, (<b>c</b>) LaFeO<sub>3</sub>, (<b>d</b>) La(Sr)FeO<sub>3</sub>; and (<b>e</b>) macro image of targets ready for microscopic examination and (<b>f</b>) the surface of the LaFeO<sub>3</sub> target after laser ablation.</p>
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<p>Laser ablation system (PLD) built with an Nd:YAG laser and the Neocera vacuum chamber, connected by an optical system (<b>a</b>). Schematic of the PLD process (<b>b</b>) and a view inside the process chamber (<b>c</b>).</p>
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<p>XRD phase analysis of (<b>a</b>) Sr-doped LaCoO<sub>3</sub> and (<b>b</b>) Sr-doped LaFeO<sub>3</sub> thin films, with JCPDS pattern cards and average crystallite sizes (estimated using the Williamson–Hall method).</p>
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<p>XPS detection/verification of chemical states of elements for La(Sr)CoO<sub>3</sub> thin films.</p>
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<p>XPS detection/verification of chemical states of elements for La(Sr)FeO<sub>3</sub> thin films.</p>
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<p>SEM images of the topography of perovskite thin films grown on monocrystalline Si substrates [001] with the result of EDS analysis of the chemical composition for (<b>a</b>) LaCoO<sub>3</sub> and (<b>b</b>) LaFeO<sub>3</sub>.</p>
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<p>SEM images of the topography of perovskite thin films grown on monocrystalline Si substrates [001] with the result of EDS analysis of the chemical composition for (<b>a</b>) Sr-doped LaCoO<sub>3</sub>, (<b>b</b>) Sr-doped LaFeO<sub>3</sub>.</p>
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<p>Surface topography images of perovskite thin films by atomic force microscopy (AFM) technique for (<b>a</b>) LaCoO<sub>3</sub> and (<b>b</b>) LaFeO<sub>3</sub>.</p>
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<p>Surface topography images of perovskite thin films by atomic force microscopy (AFM) technique for (<b>a</b>) Sr-doped LaCoO<sub>3</sub> and (<b>b</b>) Sr-doped LaFeO<sub>3</sub>.</p>
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<p>Examples of (<b>a</b>) indentation curve and (<b>b</b>) penetration depth and normal force plots obtained from nanohardness measurements of LaFeO<sub>3</sub> thin film on Si substrate.</p>
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<p>TEM analysis of LaCoO<sub>3</sub> thin films: (<b>a</b>) low-magnification bright-field image with selected area electron diffraction pattern, (<b>b</b>,<b>c</b>) high-resolution TEM images, and (<b>d</b>) SAED solved with TEM/EDS analysis.</p>
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<p>TEM analysis of Sr-doped LaCoO<sub>3</sub> thin films: (<b>a</b>,<b>b</b>,<b>d</b>,<b>e</b>) low-magnification bright- and (<b>c</b>,<b>f</b>) dark-field image with selected area electron diffraction patterns, and (<b>g</b>) SAED solved with TEM/EDS analysis.</p>
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<p>TEM analysis of LaFeO<sub>3</sub> thin films: (<b>a</b>,<b>b</b>) low-magnification bright- and (<b>c</b>) dark-field image with selected area electron diffraction pattern, (<b>d</b>,<b>e</b>) high-resolution TEM images, and (<b>f</b>) SAED solved with TEM/EDS analysis.</p>
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<p>TEM analysis of Sr-doped LaFeO<sub>3</sub> thin films: (<b>a</b>,<b>d</b>) low-magnification bright- and (<b>b</b>,<b>e</b>) dark-field image with selected area electron diffraction patterns, (<b>c</b>,<b>f</b>) high-resolution TEM images and (<b>g</b>) SAED pattern solved with TEM/EDS analysis.</p>
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<p>LaCoO<sub>3</sub> response at 500 °C exposed to 50 ppm of NO<sub>2</sub> using different currents: (<b>a</b>) 0.1 nA, (<b>b</b>) 1 nA, and (<b>c</b>) 10nA.</p>
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<p>Response of La(Sr)CoO<sub>3</sub> exposed to 50 ppm NO<sub>2</sub> at temperatures in the range of 230 ÷ 440 °C: (<b>a</b>) LaCoO<sub>3</sub>, (<b>b</b>) La<sub>0.9</sub>Sr<sub>0.1</sub>CoO<sub>3</sub>, and (<b>c</b>) La<sub>0</sub>.<sub>9</sub>Sr<sub>0.1</sub>CoO<sub>3</sub>.</p>
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<p>Response of La(Sr)CoO<sub>3</sub> exposed to 50 ppm NO<sub>2</sub> at temperatures in the range of 230 ÷ 440 °C: (<b>a</b>) LaCoO<sub>3</sub>, (<b>b</b>) La<sub>0.9</sub>Sr<sub>0.1</sub>CoO<sub>3</sub>, and (<b>c</b>) La<sub>0</sub>.<sub>9</sub>Sr<sub>0.1</sub>CoO<sub>3</sub>.</p>
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<p>Response of LaFeO<sub>3</sub> exposed to 50 ppm NO<sub>2</sub> for a range of temperatures: (<b>a</b>) 230 °C, (<b>b</b>) 300 °C, (<b>c</b>) 350 °C, (<b>d</b>) 400 °C, and (<b>e</b>) 440 °C.</p>
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<p>Response of La<sub>0</sub>.<sub>9</sub>Sr<sub>0</sub>.<sub>1</sub>FeO<sub>3</sub> exposed to 50 ppm NO<sub>2</sub> (summary chart) and for a range of temperatures: (<b>a</b>) 230 °C, (<b>b</b>) 300 °C, (<b>c</b>) 350 °C, and (<b>d</b>) 440 °C.</p>
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<p>Response of La<sub>0</sub>.<sub>8</sub>Sr<sub>0</sub>.<sub>2</sub>FeO<sub>3</sub> exposed to 50 ppm NO<sub>2</sub> (summary chart) and for a range of temperatures: (<b>a</b>) 230 °C, (<b>b</b>) 300 °C, (<b>c</b>) 350 °C, and (<b>d</b>) 440 °C.</p>
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12 pages, 4054 KiB  
Article
Low-Frequency Communication Based on Rydberg-Atom Receiver
by Yipeng Xie, Mingwei Lei, Jianquan Zhang, Wenbo Dong and Meng Shi
Electronics 2025, 14(5), 1041; https://doi.org/10.3390/electronics14051041 - 6 Mar 2025
Viewed by 146
Abstract
Rydberg-atom receivers have developed rapidly with increasing sensitivity. However, studies on their application in low-frequency electric fields remain limited. In this work, we demonstrate low-frequency communication using an electrode-embedded atom cell and a whip antenna without the need for a low-noise amplifier (LNA). [...] Read more.
Rydberg-atom receivers have developed rapidly with increasing sensitivity. However, studies on their application in low-frequency electric fields remain limited. In this work, we demonstrate low-frequency communication using an electrode-embedded atom cell and a whip antenna without the need for a low-noise amplifier (LNA). Three modulations—binary phase-shift keying (BPSK), on–off keying (OOK), and two-frequency shift keying (2FSK)—were employed for communication using a Rydberg-atom receiver operating near 100 kHz. The signal-to-noise ratio (SNR) of the modulated low-frequency signal received by Rydberg atoms was measured at various emission voltages. Additionally, we demonstrated the in-phase and quadrature (IQ) constellation diagram, error vector magnitude (EVM), and eye diagram of the demodulated signal at different symbol rates. The EVM values were measured to be 8.8% at a symbol rate of 2 kbps, 9.4% at 4 kbps, and 13.7% at 8 kbps. The high-fidelity digital color image transmission achieved a peak signal-to-noise ratio (PSNR) of 70 dB. Our results demonstrate the feasibility of a Rydberg-atom receiver for low-frequency communication applications. Full article
(This article belongs to the Topic Quantum Wireless Sensing)
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Figure 1

Figure 1
<p>Schematic of the experimental setup. An 852 nm probe laser and an identical reference beam propagated in parallel through the vapor cell, which incorporated a pair of copper electrode plates spaced 18 mm apart. A 509 nm Rydberg laser counter-propagated and overlapped with the probe laser but not the reference beam. The transmissions of the probe and reference beams were directed into a differential photodetector to measure the transmission difference. The experimental process commenced with the generation of low-frequency signals using a whip antenna connected to one of the copper plates. These signals were coupled into the vapor cell, where they interacted with the Rydberg atoms. The EIT effect was generated by the probe and Rydberg lasers, enabling the detection of low-frequency signals through changes in the probe laser transmission. The detected signals were subsequently processed using a differential photodetector and an oscilloscope for data acquisition and analysis.</p>
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<p>(<b>a</b>) EIT spectrum for the transition from intermediate state <math display="inline"><semantics> <mrow> <mo>|</mo> <mn>6</mn> <msub> <mrow> <mi>P</mi> </mrow> <mrow> <mn>3</mn> <mo>/</mo> <mn>2</mn> </mrow> </msub> <mo>,</mo> <mi>F</mi> <mo>′</mo> <mo>=</mo> <mn>5</mn> <mo>&gt;</mo> </mrow> </semantics></math> to the Rydberg state <math display="inline"><semantics> <mrow> <mo>|</mo> <mn>6</mn> <msub> <mrow> <mn>3</mn> <mi>P</mi> </mrow> <mrow> <mn>5</mn> <mo>/</mo> <mn>2</mn> </mrow> </msub> <mo>&gt;</mo> </mrow> </semantics></math>. The inset illustrates the three-level Rydberg EIT scheme. (<b>b</b>) EIT spectrum for the transition compared with a 100 kHz signal field. The inset depicts the 100 kHz signal field. (<b>c</b>) EIT spectrum for the transition compared with a DC field. (<b>d</b>) EIT spectrum for the transition compared with a 100 kHz signal field and a DC field. The inset depicts the 100 kHz signal field.</p>
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<p>(<b>a</b>) Waveforms of 2FSK, OOK, and BPSK signals. In 2FSK, the carrier signal’s frequency is modulated to represent two binary states, with distinct frequencies corresponding to ‘1’ and ‘0’. OOK is an amplitude modulation technique in which the presence of the carrier signal represents a binary ‘1’, and its absence represents a binary ‘0’. BPSK is characterized by phase modulation of the carrier signal to represent two distinct binary states, typically 0 and 1. (<b>b</b>) The generation process of the Pseudo-Random Binary Sequence (PRBS). The generation polynomial used in this work is <math display="inline"><semantics> <mrow> <mn>1</mn> <mo>+</mo> <msup> <mrow> <mi>x</mi> </mrow> <mrow> <mn>6</mn> </mrow> </msup> <mo>+</mo> <msup> <mrow> <mi>x</mi> </mrow> <mrow> <mn>7</mn> </mrow> </msup> </mrow> </semantics></math>, and the total number of bits in one period is 127.</p>
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<p>Spectrum for different modulation modes. (<b>a</b>) the OOK signal bandwidth ranged from 98 kHz to 102 kHz (<math display="inline"><semantics> <mrow> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mi>c</mi> </mrow> </msub> </mrow> </semantics></math> ± <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mi>b</mi> </mrow> </msub> </mrow> </semantics></math>); (<b>b</b>) the BPSK signal bandwidth ranged from 98 kHz to 102 kHz (<math display="inline"><semantics> <mrow> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mi>c</mi> </mrow> </msub> </mrow> </semantics></math> ± <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mi>b</mi> </mrow> </msub> </mrow> </semantics></math>); (<b>c</b>) the 2FSK signal bandwidth ranged from 88 kHz to 112 kHz (|<math display="inline"><semantics> <mrow> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msub> <mo>−</mo> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mn>1</mn> </mrow> </msub> </mrow> </semantics></math>| + 2<math display="inline"><semantics> <mrow> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mi>b</mi> </mrow> </msub> </mrow> </semantics></math>).</p>
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<p>Demodulated signal waveforms of BPSK, OOK, and 2FSK at emission voltages of 8 V, 4 V, and 1 V. (<b>a</b>) BPSK; (<b>b</b>) OOK; (<b>c</b>) 2FSK.</p>
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<p>Comparison of the SNR of the three signals as a function of the emission voltage. The SNR of the 2FSK signal received by the Rydberg atom is higher than that of OOK and BPSK. When the SNR falls below the threshold of 4 dB, demodulation of all three signal types becomes unsuccessful.</p>
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<p>IQ constellation diagrams and eye diagrams of the Rydberg atom reception at different symbol rates using BPSK modulation. (<b>a</b>) The error vector magnitude (EVM) is measured at 8.8% for a symbol rate of 2 kbps; (<b>b</b>) the EVM is measured at 9.4% for a symbol rate of 4 kbps; (<b>c</b>) the EVM is measured at 13.7% for a symbol rate of 8 kbps; (<b>d</b>) eye diagrams for a symbol rate of 2 kbps; (<b>e</b>) eye diagrams for a symbol rate of 4 kbps; (<b>f</b>) eye diagrams for a symbol rate of 8 kbps.</p>
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<p>Variation in the EVM with symbol rate for the BPSK signal received by Rydberg atoms. As the symbol rate of the BPSK signal increases, the EVM also increases, indicating a degradation of communication quality.</p>
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<p>Process of color image transmission using Rydberg atoms. The process involves six primary steps: (1) decomposing the original image into its constituent red (R), green (G), and blue (B) color spaces; (2) mapping each pixel’s intensity value to an 8-bit sequence; (3) encoding these sequences into baseband signals represented by high and low voltage levels; (4) modulating these baseband signals onto a carrier using BPSK; (5) transmitting the modulated signal; (6) demodulating the received signals to retrieve the original 8-bit sequences and reconstructing the pixel data to recover the final color image.</p>
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<p>Reception of black-and-white and color images. (<b>a</b>) Original black and white image; (<b>b</b>) received black and white image; (<b>c</b>) original color image; (<b>d</b>) received color image.</p>
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21 pages, 18398 KiB  
Article
A Low-Complexity Lossless Compression Method Based on a Code Table for Infrared Images
by Yaohua Zhu, Mingsheng Huang, Yanghang Zhu and Yong Zhang
Appl. Sci. 2025, 15(5), 2826; https://doi.org/10.3390/app15052826 - 5 Mar 2025
Viewed by 281
Abstract
Traditional JPEG series image compression algorithms have limitations in speed. To improve the storage and transmission of 14-bit/pixel images acquired by infrared line-scan detectors, a novel method is introduced for achieving high-speed and highly efficient compression of line-scan infrared images. The proposed method [...] Read more.
Traditional JPEG series image compression algorithms have limitations in speed. To improve the storage and transmission of 14-bit/pixel images acquired by infrared line-scan detectors, a novel method is introduced for achieving high-speed and highly efficient compression of line-scan infrared images. The proposed method utilizes the features of infrared images to reduce image redundancy and employs improved Huffman coding for entropy coding. The improved Huffman coding addresses the low-probability long coding of 14-bit images by truncating long codes, which results in low complexity and minimal loss in the compression ratio. Additionally, a method is proposed to obtain a Huffman code table that bypasses the pixel counting process required for entropy coding, thereby improving the compression speed. The final implementation is a low-complexity lossless image compression algorithm that achieves fast encoding through simple table lookup rules. The proposed method results in only a 10% loss in compression performance compared to JPEG 2000, while achieving a 20-fold speed improvement. Compared to dictionary-based methods, the proposed method can achieve high-speed compression while maintaining high compression efficiency, making it particularly suitable for the high-speed, high-efficiency lossless compression of line-scan panoramic infrared images. The code table compression effect is 5% lower than the theoretical value. The algorithm can also be applied to analyze images with more bits. Full article
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<p>Frequency statistics and correlation analysis of infrared images. (<b>a</b>) Original image A. (<b>b</b>) Original image A pixel frequency. (<b>c</b>) Difference image A. (<b>d</b>) Difference image A pixel frequency. (<b>e</b>) Correlation analysis of A. (<b>f</b>) Original image B. (<b>g</b>) Original image B pixel frequency. (<b>h</b>) Difference image B. (<b>i</b>) Difference image B pixel frequency. (<b>j</b>) Correlation analysis of B.</p>
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<p>Leaf node <math display="inline"><semantics> <mrow> <mo>−</mo> <mn>3</mn> </mrow> </semantics></math> backtracking towards the root node.</p>
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<p>Various experimental scenes (partial of 53).</p>
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<p>The total probability of the occurrence of pixels within the boundary pixel.</p>
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<p>Differential pixels probability distribution. (<b>a</b>) Probability distribution of the first 302 differential pixels in 53 images. (<b>b</b>) Average probability distribution of 53 images.</p>
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<p>The lossless compression algorithm. (<b>a</b>) Coding rules of the improved Huffman coding. (<b>b</b>) Framework of the lossless compression algorithm.</p>
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<p>Various experimental scenes (partial of 37).</p>
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<p>Speed and compression ratio of the proposed method and JPEG series. (<b>a</b>) Compression ratio. (<b>b</b>) Compression speed.</p>
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<p>Speed and compression ratio of the proposed method and tiff. (<b>a</b>) Compression speed. (<b>b</b>) Compression speed. (<b>c</b>) Compression ratio.</p>
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15 pages, 7261 KiB  
Article
Design of Ultra-Wide-Band Fourier Transform Infrared Spectrometer
by Liangjie Zhi, Wei Han, Shuai Yuan, Fengkun Luo, Han Gao, Zixuan Zhang and Min Huang
Optics 2025, 6(1), 7; https://doi.org/10.3390/opt6010007 - 5 Mar 2025
Viewed by 258
Abstract
A wide band range can cover more of the characteristic spectral lines of substances, and thus analyze the structure and composition of substances more accurately. In order to broaden the band range of spectral instruments, an ultra-wide-band Fourier transform infrared spectrometer is designed. [...] Read more.
A wide band range can cover more of the characteristic spectral lines of substances, and thus analyze the structure and composition of substances more accurately. In order to broaden the band range of spectral instruments, an ultra-wide-band Fourier transform infrared spectrometer is designed. The incident light of the spectrometer is constrained by a secondary imaging scheme, and switchable light sources and detectors are set to achieve an ultra-wide band coverage. A compact and highly stable double-moving mirror swing interferometer is adopted to generate optical path difference, and a controller is used to stabilize the swing of the moving mirrors. A distributed design of digital system integration and analog system integration is adopted to achieve a lightweight and low-power-consumption spectrometer. High-speed data acquisition and a transmission interface are applied to improve the real-time performance. Further, a series of experiments are performed to test the performance of the spectrometer. Finally, the experimental results show that the spectral range of the ultra-wide-band Fourier transform infrared spectrometer covers 0.770–200 μm, with an accurate wave number, a spectral resolution of 0.25 cm−1, and a signal-to-noise ratio better than 50,000:1. Full article
(This article belongs to the Section Engineering Optics)
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<p>Schematic diagram of the front optical system.</p>
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<p>Schematic diagram of the optical path of the interferometer: (<b>a</b>) double-moving mirror-swinging structure; (<b>b</b>) relationship between OPD and swing angle.</p>
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<p>Adaptive feedforward LADRC structural block diagram.</p>
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<p>Division of electronics functional units.</p>
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<p>Real-time high-speed data acquisition and transmission system.</p>
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<p>The developed ultra-wide-band FTIR spectrometer.</p>
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<p>Spectral range measurement: (<b>a</b>) FIR band; (<b>b</b>) MIR band; (<b>c</b>) NIR band.</p>
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<p>Negative-pressure CO gas cell.</p>
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<p>Absorption spectrum of CO gas.</p>
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<p>Spectrum of water vapor.</p>
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<p>SNR analysis of the proposed FTIR spectrometer.</p>
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17 pages, 12823 KiB  
Article
Remote Sensing Small Object Detection Network Based on Multi-Scale Feature Extraction and Information Fusion
by Junsuo Qu, Tong Liu, Zongbing Tang, Yifei Duan, Heng Yao and Jiyuan Hu
Remote Sens. 2025, 17(5), 913; https://doi.org/10.3390/rs17050913 - 5 Mar 2025
Viewed by 236
Abstract
Nowadays, object detection algorithms are widely used in various scenarios. However, there are further small object detection requirements in some special scenarios. Due to the problems related to small objects, such as their less available features, unbalanced samples, higher positioning accuracy requirements, and [...] Read more.
Nowadays, object detection algorithms are widely used in various scenarios. However, there are further small object detection requirements in some special scenarios. Due to the problems related to small objects, such as their less available features, unbalanced samples, higher positioning accuracy requirements, and fewer data sets, a small object detection algorithm is more complex than a general object detection algorithm. The detection effect of the model for small objects is not ideal. Therefore, this paper takes YOLOXs as the benchmark network and enhances the feature information on small objects by improving the network’s structure so as to improve the detection effect of the model for small objects. This specific research is presented as follows: Aiming at the problem of a neck network based on an FPN and its variants being prone to information loss in the feature fusion of non-adjacent layers, this paper proposes a feature fusion and distribution module, which replaces the information transmission path, from deep to shallow, in the neck network of YOLOXs. This method first fuses and extracts the feature layers used by the backbone network for prediction to obtain global feature information containing multiple-size objects. Then, the global feature information is distributed to each prediction branch to ensure that the high-level semantic and fine-grained information are more efficiently integrated so as to help the model effectively learn the discriminative information on small objects and classify them correctly. Finally, after testing on the VisDrone2021 dataset, which corresponds to a standard image size of 1080p (1920 × 1080), the resolution of each image is high and the video frame rate contained in the dataset is usually 30 frames/second (fps), with a high resolution in time, it can be used to detect objects of various sizes and for dynamic object detection tasks. And when we integrated the module into a YOLOXs network (named the FE-YOLO network) with the three improvement points of the feature layer, channel number, and maximum pool, the mAP and APs were increased by 1.0% and 0.8%, respectively. Compared with YOLOV5m, YOLOV7-Tiny, FCOS, and other advanced models, it can obtain the best performance. Full article
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<p>Two common feature fusion diagrams.</p>
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<p>Convolution and deconvolution diagram.</p>
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<p>PANet information fusion diagram.</p>
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<p>The schematic diagram of the improved neck network.</p>
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<p>Schematic diagram of FFDN module.</p>
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<p>Map of mAP0.5 during the training of Fe-YOLO and FFDN-YOLO.</p>
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<p>Comparison between FE-YOLO and FFDN-YOLO models.</p>
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<p>Comparison diagram of model detection and manual labeling.</p>
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<p>Comparison chart of detection results of different models.</p>
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<p>Variation diagram of loss value during model training.</p>
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<p>Dataset test diagram.</p>
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28 pages, 11026 KiB  
Article
Dolphin Pituitary Gland: Immunohistochemistry and Ultrastructural Cell Characterization Following a Novel Anatomical Dissection Protocol and Non-Invasive Imaging (MRI)
by Paula Alonso-Almorox, Alfonso Blanco, Carla Fiorito, Eva Sierra, Cristian Suárez-Santana, Francesco Consolli, Manuel Arbelo, Raiden Grandía Guzmán, Ignacio Molpeceres-Diego, Antonio Fernández Gómez, Javier Almunia, Ayoze Castro-Alonso and Antonio Fernández
Animals 2025, 15(5), 735; https://doi.org/10.3390/ani15050735 - 4 Mar 2025
Viewed by 384
Abstract
The pituitary gland regulates essential physiological processes in mammals. Despite its importance, research on its anatomy and ultrastructure in dolphins remains scarce. Using non-invasive imaging technology (MRI) and a novel skull-opening and dissection protocol, this study characterizes the dolphin pituitary through immunohistochemistry (IHC) [...] Read more.
The pituitary gland regulates essential physiological processes in mammals. Despite its importance, research on its anatomy and ultrastructure in dolphins remains scarce. Using non-invasive imaging technology (MRI) and a novel skull-opening and dissection protocol, this study characterizes the dolphin pituitary through immunohistochemistry (IHC) and transmission electron microscopy (TEM). A total of 47 pituitaries were collected from stranded common bottlenose dolphins (Tursiops truncatus). common dolphins (Delphinus delphis), and Atlantic spotted dolphins (Stenella frontalis). as well as from captive common bottlenose dolphins. MRI allowed visualization of the gland’s anatomy and its spatial relationship with the hypothalamus and surrounding structures. A modified skull-opening and pituitary extraction protocol ensured the preservation of the adenohypophysis and neurohypophysis for detailed analysis. Histological, immunohistochemical, and ultrastructural studies confirmed the gland’s structural organization, identifying eight distinct adenohypophyseal cell types: corticotrophs (ACTH), somatotrophs (GH), gonadotrophs (FSH and LH), lactotrophs (LTH), melanotrophs (MSH), thyrotrophs (TSH), follicular cells, and capsular cells. This study presents the first immunolabelling of thyrotrophs in cetacean adenohypophysis and the first detailed ultrastructural characterization of adenohypophyseal cells in cetaceans, providing baseline data for future research. By integrating multidisciplinary techniques, it advances the understanding of dolphin neuroendocrinology and highlights broader implications for cetacean health, welfare, and conservation. Full article
(This article belongs to the Section Wildlife)
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<p>Modified skull-opening protocol for dolphins. The image shows a caudal view (<b>A</b>), ventral view (<b>B</b>), and lateral view (<b>C</b>) of the dolphin’s skulls. Dorsal line (blue), lateral lines (yellow), and ventral continuation lines (red). Images edited from Cozzi and Elsberry [<a href="#B23-animals-15-00735" class="html-bibr">23</a>,<a href="#B24-animals-15-00735" class="html-bibr">24</a>].</p>
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<p>(<b>A</b>) T2-weighted MRI coronal section of a dolphin’s head showing major brain structures. The pituitary gland (red arrow) is located at the base of the brain, above the sphenoid bone and ventral to the hypothalamus. It appears as a small, well-defined structure with intermediate signal intensity, framed by the bilateral optic tracts. (<b>B</b>) T2-weighted MRI sagittal section of a dolphin’s head showing major brain structures. The pituitary gland (red arrow) is located caudal to the optic chiasm (white arrow). The cerebrospinal fluid in the ventricles (asterisk) is visible with high signal intensity.</p>
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<p>Macroscopic and microscopic sagittal views of a common dolphin’s pituitary gland. (<b>A</b>) Formalin-fixed common dolphin’s brain showing the hypothalamus, optic chiasm, and pituitary gland. The adenohypophysis (white asterisk) is located cranio-ventrally to the neurohypophysis (black asterisk). The infundibular stalk connecting the hypophysis to the hypothalamus is also apparent (red arrow). (<b>B</b>) Histological view stained with H-E at 4× magnification. Both the neurohypophysis (black asterisk) and the adenohypophysis in its <span class="html-italic">pars distalis</span> (white asterisk) are observed. The adenohypophysis is continued by its <span class="html-italic">pars tuberalis</span> at the infundibular stalk level (red arrow). The neuroendocrine connection between the endocrine tissue and nervous tissue is clearly demarcated.</p>
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<p>Histological and histochemical characterization of the pituitary gland in delphinid species. (<b>A</b>) Masson’s Trichrome (MT) staining at 4× magnification in a common bottlenose dolphin. The adenohypophysis (asterisk) and neurohypophysis (triangle) are distinctly separated by a thick band of dura mater and connective tissue; a highly vascular rete-like structure envelops the gland (arrow). The inset shows the neurohypophysis (MT) at 40× magnification with structures compatible with Herring bodies (arrow). (<b>B</b>) Hematoxylin-Eosin (H-E) staining at 40× magnification of the adenohypophysis of an Atlantic spotted dolphin. Acidophils, basophils, and chromophobes are arranged in cell clusters. The inset shows the same region stained with PAS-OG. (<b>C</b>) High-magnification (40×) view of the neurohypophysis in a common dolphin, stained with H-E. The image reveals unmyelinated axons, pituicytes, and structures compatible with Herring bodies (arrow). (<b>D</b>) H-E stained pituitary gland of a newborn common bottlenose dolphin at 4× magnification. The image shows the highly vascularized <span class="html-italic">pars tuberalis</span> and subjacent <span class="html-italic">pars distalis</span>.</p>
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<p>Immunohistochemical characterization of adenohypophyseal cell populations in common bottlenose dolphins using specific antibodies to anti-ACTH at 4× magnification. ACTH-positive cells exhibit strong cytoplasmic labelling and are individually dispersed or organized in small groups within the adenohypophysis. The inset provides a higher magnification (40×) view, highlighting the distinct labelling pattern in the cytoplasm of ACTH-expressing cells.</p>
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<p>Immunohistochemical characterization of adenohypophyseal cell populations in common bottlenose dolphins using specific antibodies to anti-MSH antibody at 4× magnification. MSH-positive cells are distributed throughout the adenohypophysis, following the arrangement of endocrine cords. Cytoplasmic staining is evident. The inset shows a 40× magnification, offering a detailed view of the cytoplasmic labelling.</p>
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<p>Immunohistochemical characterization of TSH-producing cells in common bottlenose dolphins. The image shows a 40× magnification, highlighting TSH-positive cells scattered individually throughout the adenohypophysis. TSH-positive cells exhibit a polygonal shape with distinct cytoplasmic staining. The inset (40× magnification) presents another region of the gland, confirming the dispersed distribution pattern of TSH-expressing cells.</p>
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<p>Schematic representation of the general morphology and ultrastructural characteristics (overall cellular and nuclear shape and size, secretion granules size and density, nucleus, rough endoplasmatic reticulum, Golgi complex, mitochondria) of the six different hormone-producing endocrine cells in the common dolphin (<span class="html-italic">Delphinus delphis</span>) pituitary gland. (<b>A</b>) Corticotrophs (<b>B</b>) Lactotrophs, (<b>C</b>) Somatotrophs, (<b>D</b>) Gonadotrophs, (<b>E</b>) Thyrotrophs, and (<b>F</b>) Melanotrophs. The illustration highlights key morphological and ultrastructural features of each cell type, as described in the text. Created in BioRender, version 04.</p>
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<p>Transmission electron microscopy images of the adenohypophysis structure and identification of different hormone-producing cells in common dolphins (<span class="html-italic">Delphinus delphis</span>). Abbreviations: A.C.T.H., corticotrophs; L.T.H., lactotrophs, Gh, somatotrophs, T.S.H., thyrotrophs.</p>
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<p>Transmission electron microscopy images of ACTH-producing cells in common dolphins <span class="html-italic">(Delphinus delphis)</span>. (<b>A</b>) The cell shows a large central nucleus with a visible nucleolus (arrow). (<b>B</b>) ACTH cytoplasmic projection with aligned granules in the cell membrane. (<b>C</b>) Abundant rough endoplasmic reticulum arranged in concentric layers (arrow). (<b>D</b>) Aligned ACTH electrodense granules along the cytoplasmic membrane (arrow), prepared for secretion.</p>
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<p>Transmission electron microscopy images of LTH-producing cells in common dolphins (Delphinus delphis). (<b>A</b>) The cell exhibits an ovoid morphology, characteristic of LTH-producing cells (arrow). (<b>B</b>) Presence of centrioles, which play a role in intracellular transport and cellular organization (arrow). (<b>C</b>) The cytoplasm contains highly pleomorphic granules, varying in size and shape, indicative of secretory activity (arrow). (<b>D</b>) A well-developed Golgi complex is observed (arrow); mitochondria are also abundant.</p>
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<p>Transmission electron microscopy images of GH-producing cells in common dolphins (<span class="html-italic">Delphinus delphis</span>). (<b>A</b>) The cytoplasm contains abundant granules distributed throughout (arrow). The cell exhibits an ovoid morphology (arrow), a typical feature of somatotrophs. (<b>B</b>) Large, spherical, electron-dense granules are closely attached to the cytoplasmic membrane (arrow), suggesting active secretion. (<b>C</b>) A well-developed Golgi complex occupies a large cytoplasmic area (arrow), reflecting its role in processing and packaging secretory granules. (<b>D</b>) The nucleus appears spherical with a prominent nucleolus (arrow).</p>
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<p>Transmission electron microscopy images of GnRH-producing (gonadotroph) cells in common dolphins (<span class="html-italic">Delphinus delphis</span>). (<b>A</b>) The cell exhibits an ovoid shape with a centralized nucleus. (<b>B</b>) A pleomorphic nucleus is observed (arrow), indicating nuclear variability in these endocrine cells. (<b>C</b>) A well-developed Golgi complex is prominent, reflecting its role in hormone processing and packaging. (<b>D</b>) Dilated rough endoplasmic reticulum cisternae with homogeneous content are evident (arrow), suggesting active protein synthesis. Additionally, numerous mitochondria are present throughout the cytoplasm.</p>
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<p>Transmission electron microscopy images of thyrotrophs in common dolphins (<span class="html-italic">Delphinus delphis</span>). (<b>A</b>) The cell exhibits an ovoid shape at low magnification (arrow). (<b>B</b>) Dilated rough endoplasmic reticulum cisternae are observed, appearing as sac-like structures with clear, homogeneous content (arrow). (<b>C</b>) Numerous mitochondria, particularly with a lamellar structure (arrow), are present, suggesting high metabolic activity. (<b>D</b>) Medium-sized granules are distributed within the cytoplasm.</p>
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<p>Transmission electron microscopy images of MSH-producing cells in a common dolphin (<span class="html-italic">Delphinus delphis</span>). (<b>A</b>) The cell exhibits an ovoid shape. Abundant granules with varying content are visible within the cytoplasm. (<b>B</b>) Myelin figures are observed (arrow). (<b>C</b>) Large lysosomes are present (arrow), likely involved in cellular digestion and turnover. (<b>D</b>) A well-developed Golgi complex with numerous flattened sacs is observed (arrow), involved in processing and packaging hormones. Additionally, mitochondria are present throughout the cytoplasm, indicating high metabolic activity.</p>
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<p>Transmission electron microscopy images of follicular and capsular cells in the adenohypophysis of common dolphins (<span class="html-italic">Delphinus delphis</span>). (<b>A</b>) Desmosomes are visible between the follicular cells, suggesting cell–cell adhesion (arrow). (<b>B)</b> A follicular cavity is observed, characteristic of the structure of these cells (arrow). (<b>C</b>) In capsular cells, the presence of fat droplets is evident, indicating lipid storage (arrow). Additionally, the capsular cells form a thin lining around the adenohypophysis. (<b>D</b>) The capsular cells are arranged in a pseudoepithelial palisade (arrow).</p>
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18 pages, 3903 KiB  
Article
Lossless Hyperspectral Image Compression in Comet Interceptor and Hera Missions with Restricted Bandwith
by Kasper Skog, Tomáš Kohout, Tomáš Kašpárek, Antti Penttilä, Monika Wolfmayr and Jaan Praks
Remote Sens. 2025, 17(5), 899; https://doi.org/10.3390/rs17050899 - 4 Mar 2025
Viewed by 169
Abstract
Lossless image compression is vital for missions with limited data transmission bandwidth. Reducing file sizes enables faster transmission and increased scientific gains from transient events. This study compares two wavelet-based image compression algorithms, CCSDS 122.0 and JPEG 2000, used in the European Space [...] Read more.
Lossless image compression is vital for missions with limited data transmission bandwidth. Reducing file sizes enables faster transmission and increased scientific gains from transient events. This study compares two wavelet-based image compression algorithms, CCSDS 122.0 and JPEG 2000, used in the European Space Agency Comet Interceptor and Hera missions, respectively, in varying scenarios. The JPEG 2000 implementation is sourced from the JasPer library, whereas a custom implementation was written for CCSDS 122.0. The performance analysis for both algorithms consists of compressing simulated asteroid images in the visible and near-infrared spectral ranges. In addition, all test images were noise-filtered to study the effect of the amount of noise on both compression ratio and speed. The study finds that JPEG 2000 achieves consistently higher compression ratios and benefits from decreased noise more than CCSDS 122.0. However, CCSDS 122.0 produces comparable results faster than JPEG 2000 and is substantially less computationally complex. On the contrary, JPEG 2000 allows dynamic (entropy-permitting) reduction in the bit depth of internal data structures to 8 bits, halving the memory allocation, while CCSDS 122.0 always works in 16-bit mode. These results contribute valuable knowledge to the behavioral characteristics of both algorithms and provide insight for entities planning on using either algorithm on board planetary missions. Full article
(This article belongs to the Section Remote Sensing Image Processing)
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<p>The OPIC (<b>left</b>) and EnVisS (<b>right</b>) cameras of the Comet Interceptor mission, modified [<a href="#B1-remotesensing-17-00899" class="html-bibr">1</a>].</p>
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<p>ASPECT camera of the Hera mission.</p>
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<p>A flowchart of the simulated data set creation. The software consists of three parts and the second and third part take the output of the previous part as input, together with additional parameters. Python version used is 3.10, Blender 3.6, and AIS 0.9.</p>
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<p>Simulated test images indexed with their corresponding simulation parameters.</p>
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<p>Differential encoding of a hyperspectral datacube example. First wavelength compressed normally (<b>left</b>) and subsequent differentially encoded wavelengths (<b>middle</b>) and (<b>right</b>).</p>
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<p>Images used to find edge cases in the CCSDS 122.0 image compression algorithm. From left to right: white noise, pure black, smooth gradient and vertical stripes.</p>
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<p>NIR Image 1 with 40 ms exposure time (<b>top left</b>), NIR image 1 noiseless (<b>top right</b>) and the difference between noisy and noiseless (<b>bottom</b>).</p>
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<p>Example of the compression ratio plots for indexed Vis and NIR images (<b>bottom</b>) with three exposure times per image: 5 ms, 10 ms and 20 ms for Vis (<b>top left</b>) and 10 ms, 20 ms and 40 ms for NIR (<b>top right</b>). All images are shown with and without FORPDN filtering.</p>
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<p>Performance of the CCSDS 122.0 and JPEG 2000 compression algorithms on three exposure levels of the noiseless, noisy and filtered visible spectrum images. Filtering is performed with FORPDN, HyRes, LRMR and W3D.</p>
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<p>Performance of the CCSDS 122.0 and JPEG 2000 compression algorithms on three exposure levels of the noiseless, noisy and filtered differentially encoded visible spectrum images. Filtering is performed with FORPDN, HyRes, LRMR and W3D.</p>
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<p>The entropy of three exposure levels of noisy Vis and NIR images (<b>left</b>) and their noiseless variants (<b>right</b>).</p>
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<p>Performance of the CCSDS 122.0 and JPEG 2000 compression algorithms on three exposure levels of filtered and noisy near-infrared images. Filtering is performed with FORPDN, HyRes, LRMR and W3D.</p>
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<p>The performance of the CCSDS 122.0 and JPEG 2000 compression algorithms on three exposure levels of filtered and noisy differentially encoded near-infrared images. Filtering is performed with FORPDN, HyRes, LRMR and W3D.</p>
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18 pages, 4314 KiB  
Article
MMI Couplers and the Talbot Effect, Symmetries and Golden Ratio
by Gazi Mahamud Hasan, Mehedi Hasan, Karin Hinzer and Trevor Hall
Photonics 2025, 12(3), 229; https://doi.org/10.3390/photonics12030229 - 3 Mar 2025
Viewed by 238
Abstract
The Talbot effect concerns the periodic self-imaging along an optical axis of a free-space optical field that is periodic in an initial transverse plane. It may be modeled by a shift-invariant linear system, fully characterized by the convolution of its impulse response. Self-imaging [...] Read more.
The Talbot effect concerns the periodic self-imaging along an optical axis of a free-space optical field that is periodic in an initial transverse plane. It may be modeled by a shift-invariant linear system, fully characterized by the convolution of its impulse response. Self-imaging at integer and fractional Talbot distances of point sources on a regular grid in free space may then be represented by a transmission matrix that is circulant, symmetric, and persymmetric. The free-space Talbot effect may be mapped to the Talbot effect in a multimode waveguide by imposing the anti-symmetry of the mirror-like sidewalls created by the tight confinement of light within a high-index contrast multimode waveguide. The position of the anti-symmetry axis controls the distribution of discrete lattice points in a unit cell. For different distributions, interesting features such as conditional flexibility in the placement of access ports without altering amplitude and phase relationships, omitting ports without power penalty, closed form uneven splitting ratios, and offset access ports can be derived from the MMI coupler. As a specific example, a simple 2×2 MMI coupler is shown to provide a power-splitting ratio related to the golden ratio φ. The structure is amenable to planar photonic integration on any high-index contrast platform. The predictions of the theory are confirmed by simulation and verified by experimental measurements on a golden ratio MMI coupler fabricated using an SOI process. Full article
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<p>(<b>a</b>) Free-space Talbot effect with diffraction grating illuminated by coherent light with wavelength λ. Shifted (blue) and direct (red) single replicas of the illuminated grating are observed at odd multiples of <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>z</mi> </mrow> <mrow> <mi>T</mi> </mrow> </msub> </mrow> </semantics></math> and even multiples of <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>z</mi> </mrow> <mrow> <mi>T</mi> </mrow> </msub> </mrow> </semantics></math> distances, respectively. Multiple self-images formed at a rational fractional multiple of <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>z</mi> </mrow> <mrow> <mi>T</mi> </mrow> </msub> </mrow> </semantics></math> are not shown. Sharp images can be achieved with a grating with infinitely many slits and a period consistent with the paraxial approximation Λ &gt;&gt; λ. In the case of an infinite grating and lossless free space, the image field will be periodic in both transverse and longitudinal coordinates; (<b>b</b>) the arrangement of the illuminating source and image field into their corresponding delta distribution at lattice points with pitch <math display="inline"><semantics> <mrow> <mrow> <mrow> <mo>Λ</mo> </mrow> <mo>/</mo> <mrow> <mn>2</mn> <mi>q</mi> </mrow> </mrow> </mrow> </semantics></math>. Vectors <math display="inline"><semantics> <mrow> <mi mathvariant="bold-italic">a</mi> </mrow> </semantics></math> and <math display="inline"><semantics> <mrow> <mi mathvariant="bold-italic">b</mi> </mrow> </semantics></math> provide a complete description of the distribution; and (<b>c</b>) the transformation due to Talbot effect. The periodic input, Talbot effect impulse response, and output distributions are arranged by wrapping their common period around a circle, and thus convolution is modified to circular convolution.</p>
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<p>An arrangement of a multimode waveguide section to exploit the free-space Talbot effect analysis of its transmission characteristics. The section that exists is the physical multimode waveguide section with width <math display="inline"><semantics> <mrow> <mi>W</mi> </mrow> </semantics></math>. The core-cladding boundaries with high refractive index contrast act as mirrors and thus introduce anti-symmetry. Type I anti-symmetry is imposed by placing the anti-symmetry axis midway between two lattice points. The ideal mirrors provide an infinite number of replications and thus virtual multimode waveguide is formed. A unit cell with period <math display="inline"><semantics> <mrow> <mo>Λ</mo> </mrow> </semantics></math> is formed with two such sections.</p>
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<p>(<b>a</b>) The Talbot carpet generated by a point source in a unit cell with a longitudinal dimension <math display="inline"><semantics> <mrow> <mi>z</mi> <mo>=</mo> <msub> <mrow> <mi>z</mi> </mrow> <mrow> <mi>T</mi> </mrow> </msub> </mrow> </semantics></math>. The physically existing point source is at the lattice point <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msub> </mrow> </semantics></math>. The boundary mirrors the physical section into a virtual section, which constitutes the unit cell. Zoomed-in versions of the Talbot carpet depicting only the physical multimode section with image plane at <math display="inline"><semantics> <mrow> <mi>z</mi> <mo>=</mo> <mstyle scriptlevel="0" displaystyle="true"> <mfrac> <mrow> <mn>1</mn> </mrow> <mrow> <mn>3</mn> </mrow> </mfrac> </mstyle> <msub> <mrow> <mi>z</mi> </mrow> <mrow> <mi>T</mi> </mrow> </msub> </mrow> </semantics></math> and source at lattice points (<b>b</b>) <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>1</mn> </mrow> </msub> </mrow> </semantics></math>, (<b>c</b>) <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msub> </mrow> </semantics></math>, and (<b>d</b>) <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>5</mn> </mrow> </msub> </mrow> </semantics></math>.</p>
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<p>Type II anti-symmetry imposed by the positioning the axis of anti-symmetry through a lattice point. The breaking of translation symmetry ensures a zero field at these points, and thus no physical access port is possible at <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>0</mn> </mrow> </msub> </mrow> </semantics></math> and <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mo>±</mo> <mi>q</mi> </mrow> </msub> </mrow> </semantics></math>.</p>
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<p>(<b>a</b>) Schematic of a golden ratio MMI coupler. Only two lattice points are equipped with tapered access ports at input (<math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msub> </mrow> </semantics></math> and <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>4</mn> </mrow> </msub> </mrow> </semantics></math>) and output (<math display="inline"><semantics> <mrow> <msub> <mrow> <mi>b</mi> </mrow> <mrow> <mn>1</mn> </mrow> </msub> </mrow> </semantics></math> and <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>b</mi> </mrow> <mrow> <mn>3</mn> </mrow> </msub> </mrow> </semantics></math>) sides. The red lattice points remain unoccupied; (<b>b</b>) The field profile through the multimode section simulated by FIMMPROP optical propagation tool. Light is launched through the access port at lattice point <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>a</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msub> </mrow> </semantics></math>. The propagation through the tapered sections is not shown.</p>
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<p>(<b>a</b>) Micrograph of the golden ratio MMI coupler and Mach–Zehnder delay interferometer with two golden ratio MMI couplers; (<b>b</b>) schematic of experimental setup.</p>
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<p>Measured ratio of intensity of light at two output ports captured by the power sensor is compared with the ideal ratio <math display="inline"><semantics> <mrow> <msup> <mrow> <mi>φ</mi> </mrow> <mrow> <mn>2</mn> </mrow> </msup> <mo>:</mo> <mn>1</mn> </mrow> </semantics></math>.</p>
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<p>(<b>a</b>) Numerical and (<b>b</b>) measured optical transmission of Mach–Zehnder delay interferometer (MZDI) with two golden ratio MMI coupler.</p>
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23 pages, 3252 KiB  
Review
Intrauterine Zika Virus Infection: An Overview of the Current Findings
by Ana Luiza Soares dos Santos, Beatriz Bussi Rosolen, Fernanda Curvelo Ferreira, Isabella Samões Chiancone, Stefany Silva Pereira, Karina Felippe Monezi Pontes, Evelyn Traina, Heron Werner, Roberta Granese and Edward Araujo Júnior
J. Pers. Med. 2025, 15(3), 98; https://doi.org/10.3390/jpm15030098 - 1 Mar 2025
Viewed by 328
Abstract
Zika virus (ZIKV) is a mosquito-borne flavivirus of the family Flaviviridae. The association between ZIKV and microcephaly was first described in Brazil in 2015. The risk of vertical transmission occurs in pregnant women with or without symptoms, and the risk of malformation appears [...] Read more.
Zika virus (ZIKV) is a mosquito-borne flavivirus of the family Flaviviridae. The association between ZIKV and microcephaly was first described in Brazil in 2015. The risk of vertical transmission occurs in pregnant women with or without symptoms, and the risk of malformation appears to be worse when infection occurs in the first and second trimesters of pregnancy. The rate of vertical transmission varies from 26 to 65%, and not all fetuses develop malformations. The incidence of malformations resulting from transmission is uncertain, ranging from 6–8% in the US to 40% in Brazil. Congenital ZIKV syndrome is a set of clinical manifestations that can affect the fetus of a mother infected with ZIKV. The manifestations are broad and nonspecific, including microcephaly, subcortical calcifications, ocular changes, congenital contractures, early hypertension, and pyramidal and extrapyramidal signs. Other findings such as growth restriction and fetal miscarriage/death may also occur. Our aim in this article is to review the literature on mosquito transmission, clinical presentation, serologic diagnosis, intrauterine transmission, pre- and postnatal imaging diagnostic findings, and short- and long-term follow-up. Full article
(This article belongs to the Section Epidemiology)
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<p>Zika virus sylvatic and urban transmission cycles.</p>
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<p>Prenatal ultrasound (37 weeks) axial view findings showing periventricular calcifications (arrows) and ventricular dilatation (*). Note normal cerebellum.</p>
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<p>Magnetic resonance imaging axial T2-weighted and diffusion-weighted magnetic resonance imaging at 37 weeks, showing ventricular dilatation (*) and smoothness of the brain surface (arrow). Note normal cerebellum.</p>
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<p>Coronal and sagittal plane (T2-weighted magnetic resonance imaging) showing smoothness of the brain surface (white arrow). Note microcephaly and redundant skin fold (black arrow). Ventricular dilatation is clearly seen in the coronal plane (*).</p>
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<p>Postnatal computed tomography scan showing parenchymal atrophy, microcephaly, widespread/multiple brain calcifications (arrows), and ventricular dilatation (*).</p>
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19 pages, 10608 KiB  
Article
Urban Waterlogging Monitoring and Recognition in Low-Light Scenarios Using Surveillance Videos and Deep Learning
by Jian Zhao, Xing Wang, Cuiyan Zhang, Jing Hu, Jiaquan Wan, Lu Cheng, Shuaiyi Shi and Xinyu Zhu
Water 2025, 17(5), 707; https://doi.org/10.3390/w17050707 - 28 Feb 2025
Viewed by 250
Abstract
With the intensification of global climate change, extreme precipitation events are occurring more frequently, making the monitoring and management of urban flooding a critical global issue. Urban surveillance camera sensor networks, characterized by their large-scale deployment, rapid data transmission, and low cost, have [...] Read more.
With the intensification of global climate change, extreme precipitation events are occurring more frequently, making the monitoring and management of urban flooding a critical global issue. Urban surveillance camera sensor networks, characterized by their large-scale deployment, rapid data transmission, and low cost, have emerged as a key complement to traditional remote sensing techniques. These networks offer new opportunities for high-spatiotemporal-resolution urban flood monitoring, enabling real-time, localized observations that satellite and aerial systems may not capture. However, in low-light environments—such as during nighttime or heavy rainfall—the image features of flooded areas become more complex and variable, posing significant challenges for accurate flood detection and timely warnings. To address these challenges, this study develops an imaging model tailored to flooded areas under low-light conditions and proposes an invariant feature extraction model for flooding areas within surveillance videos. By using extracted image features (i.e., brightness and invariant features of flooded areas) as inputs, a deep learning-based flood segmentation model is built on the U-Net architecture. A new low-light surveillance flood image dataset, named UWs, is constructed for training and testing the model. The experimental results demonstrate the efficacy of the proposed method, achieving an mRecall of 0.88, an mF1_score of 0.91, and an mIoU score of 0.85. These results significantly outperform the comparison algorithms, including LRASPP, DeepLabv3+ with MobileNet and ResNet backbones, and the classic DeepLabv3+, with improvements of 4.9%, 3.0%, and 4.4% in mRecall, mF1_score, and mIoU, respectively, compared to Res-UNet. Additionally, the method maintains its strong performance in real-world tests, and it is also effective for daytime flood monitoring, showcasing its robustness for all-weather applications. The findings of this study provide solid support for the development of an all-weather urban surveillance camera flood monitoring network, with significant practical value for enhancing urban emergency management and disaster reduction efforts. Full article
(This article belongs to the Section Urban Water Management)
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<p>The infrared images of the surveillance camera. (<b>a</b>–<b>d</b>) show the changes in the water features before and after the car drives by. (<b>e</b>–<b>h</b>) show the changes in water features at different surveillance camera positions and attitudes. The flooding area is labeled in red.</p>
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<p>False color images of the surveillance camera. (<b>a</b>–<b>d</b>) show the changes in the water features before and after a car drives by. (<b>e</b>–<b>h</b>) show the variation in water features at different surveillance camera positions and poses. The flooding area is labeled in red.</p>
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<p>Architecture of Aunet. The Dis<sub>LA</sub> module realizes the separation of the invariant features of the flooding area of the low-light scene, and the U-Net [<a href="#B43-water-17-00707" class="html-bibr">43</a>] network realizes the segmentation of the flooding region of the low-light scene. The white areas represent flood.</p>
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<p>Dis<sub>LA</sub> composition of the module, where 7 × 7 @128 denotes that there are 128 sets of convolutional kernels of the size 7 × 7. * [N, H, W, C] denotes the input dimension of the module, where N is the Batchsize, H is the height, W is the width, and C is the number of channels.</p>
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<p>The architecture of the Swin Transformer block [<a href="#B47-water-17-00707" class="html-bibr">47</a>].</p>
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<p>Some surveillance scenarios within the constructed dataset.</p>
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<p>Segmentation effect of floods for each model in the black-and-white image. The red areas represent floods. The green-framed areas are of particular interest.</p>
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<p>Segmentation effect of flooding areas for each model in the false color image. The red areas represent floods. The green, yellow, and blue-framed areas are of particular interest.</p>
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<p>Effect of Aunet and comparison models on negative samples (water-free regions at night). The red areas represent floods.</p>
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<p>Aunet and comparison modeling of flooding area segmentation effect in daytime flood images. The red areas represent floods.</p>
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16 pages, 10553 KiB  
Article
Study on the Grain Growth Behavior of Ultra-High Strength Stainless Steel
by Xiaohui Wang, Zhenbao Liu, Jiahao Chen, Jianxiong Liang, Zhiyong Yang, Wenyu Zhao and Shuai Tian
Materials 2025, 18(5), 1064; https://doi.org/10.3390/ma18051064 - 27 Feb 2025
Viewed by 148
Abstract
In this work, we aimed to study the austenite grain growth behavior of an ultra-high-strength stainless steel within the temperature range of 900–1150 °C and holding time range of 0–120 min, using a metallographic microscope and metallographic image analysis software to perform a [...] Read more.
In this work, we aimed to study the austenite grain growth behavior of an ultra-high-strength stainless steel within the temperature range of 900–1150 °C and holding time range of 0–120 min, using a metallographic microscope and metallographic image analysis software to perform a statistical analysis of grain size variation. The undissolved phases of the steel were investigated using a field emission scanning electron microscope (SEM) and transmission electron microscope (TEM). Within the temperature range of 900–950 °C, the grain growth rate of the steel was slow, while within the range of 1000–1150 °C, the grain growth rate was relatively fast. This is attributed to the precipitation of a large number of M6C-type carbides during the forging and annealing processes. In the temperature range of 900–950 °C, the solid solubility of the M6C phase was low and the pinning effect was significant, which hindered the growth of austenite grains. Above 950 °C, the carbides were dissolved extensively, weakening the pinning effect on the grain boundaries and accelerating the grain growth rate. A predictive mathematical model for the growth of the original austenite grains was established based on the Arrhenius equation, elucidating the effects of heating temperature, holding time, initial grain size, and number of carbides on the growth of austenite grains, providing a theoretical basis for heat treatment process design in actual production. Full article
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Figure 1
<p>Schematic diagram of the austenite grain growth experimental process.</p>
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<p>Morphology and grain size statistics of the original austenite grains after the temperature was held at 950 °C for different durations: (<b>a</b>) 0 min, (<b>b</b>) 5 min, (<b>c</b>) 10 min, (<b>d</b>) 30 min, (<b>e</b>) 60 min, and (<b>f</b>) 90 min. (There is no obvious change in the size of the original austenite grains).</p>
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<p>Morphology and grain size statistics of the original austenite grains after the temperature was held at 950 °C for different durations: (<b>a</b>) 0 min, (<b>b</b>) 5 min, (<b>c</b>) 10 min, (<b>d</b>) 30 min, (<b>e</b>) 60 min, and (<b>f</b>) 90 min. (There is no obvious change in the size of the original austenite grains).</p>
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<p>Morphology and grain size statistics of the original austenite grains after the temperature was held at 1050 °C for different durations: (<b>a</b>) 0 min, (<b>b</b>) 5 min, (<b>c</b>) 10 min, (<b>d</b>) 30 min, (<b>e</b>) 60 min, and (<b>f</b>) 90 min. (As the holding time increased, the mixed grain structure disappeared, and the grains began to coarsen).</p>
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<p>Morphology and grain size statistics of the original austenite grains after the temperature was held at 1150 °C for different durations: (<b>a</b>) 0 min, (<b>b</b>) 5 min, (<b>c</b>) 10 min, (<b>d</b>) 30 min, (<b>e</b>) 60 min, and (<b>f</b>) 90 min. (The grains began to grow significantly after the holding time started, and the size was significantly coarsened).</p>
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<p>The evolution of the original austenite grain size with heating temperature at different holding times.</p>
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<p>The evolution of the original austenite grain size with holding time at different holding temperatures.</p>
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<p>Microstructure of steel after different heating temperatures and holding times: (<b>a</b>) 950 °C for 5 min, (<b>b</b>) 950 °C for 60 min, (<b>c</b>) 950 °C for 120 min, (<b>d</b>) 1050 °C for 10 min, (<b>e</b>) 1050 °C for 60 min, (<b>f</b>) 1050 °C for 90 min, (<b>g</b>) 1150 °C for 5 min, and (<b>h</b>) 1150 °C for 15 min.</p>
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<p>TEM micrographs and selected-area electron diffraction patterns of larger M<sub>6</sub>C carbides. (<b>a</b>) bright-field image, (<b>b</b>) selected-area electron diffraction patterns.</p>
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<p>The relationship curves of <math display="inline"><semantics> <mrow> <mi>ln</mi> <mo> </mo> <mo>(</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mi>t</mi> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>−</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mn>0</mn> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>)</mo> </mrow> </semantics></math> and lnt at holding temperatures of 900–950 °C: (<b>a</b>) n = 0.5, (<b>b</b>) n = 1.0, (<b>c</b>) n = 1.5, (<b>d</b>) n = 2.0, (<b>e</b>) n = 2.5, and (<b>f</b>) n = 3.0.</p>
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<p>The relationship curves of <math display="inline"><semantics> <mrow> <mi>ln</mi> <mo> </mo> <mo>(</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mi>t</mi> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>−</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mn>0</mn> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>)</mo> </mrow> </semantics></math> and lnt at holding temperatures of 1000–1150 °C: (<b>a</b>) n = 0.5, (<b>b</b>) n = 1.0, (<b>c</b>) n = 1.5, (<b>d</b>) n = 2.0, (<b>e</b>) n = 2.5, and (<b>f</b>) n = 3.0.</p>
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<p>The relationship curves of <math display="inline"><semantics> <mrow> <mi>ln</mi> <mo> </mo> <mo>(</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mi>t</mi> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>−</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mn>0</mn> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>)</mo> </mrow> </semantics></math> and 1/T at holding temperatures of 900–950 °C: (<b>a</b>) n = 0.5, (<b>b</b>) n = 1.0, (<b>c</b>) n = 1.5, (<b>d</b>) n = 2.0, (<b>e</b>) n = 2.5, and (<b>f</b>) n = 3.0.</p>
Full article ">Figure 11 Cont.
<p>The relationship curves of <math display="inline"><semantics> <mrow> <mi>ln</mi> <mo> </mo> <mo>(</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mi>t</mi> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>−</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mn>0</mn> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>)</mo> </mrow> </semantics></math> and 1/T at holding temperatures of 900–950 °C: (<b>a</b>) n = 0.5, (<b>b</b>) n = 1.0, (<b>c</b>) n = 1.5, (<b>d</b>) n = 2.0, (<b>e</b>) n = 2.5, and (<b>f</b>) n = 3.0.</p>
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<p>The relationship curves of <math display="inline"><semantics> <mrow> <mi>ln</mi> <mo> </mo> <mo>(</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mi>t</mi> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>−</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mn>0</mn> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>)</mo> </mrow> </semantics></math> and 1/T at holding temperatures of 1000–1150 °C: (<b>a</b>) n = 0.5, (<b>b</b>) n = 1.0, (<b>c</b>) n = 1.5, (<b>d</b>) n = 2.0, (<b>e</b>) n = 2.5, and (<b>f</b>) n = 3.0.</p>
Full article ">Figure 12 Cont.
<p>The relationship curves of <math display="inline"><semantics> <mrow> <mi>ln</mi> <mo> </mo> <mo>(</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mi>t</mi> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>−</mo> <msubsup> <mrow> <mi mathvariant="normal">d</mi> </mrow> <mrow> <mn>0</mn> </mrow> <mrow> <mi>n</mi> </mrow> </msubsup> <mo>)</mo> </mrow> </semantics></math> and 1/T at holding temperatures of 1000–1150 °C: (<b>a</b>) n = 0.5, (<b>b</b>) n = 1.0, (<b>c</b>) n = 1.5, (<b>d</b>) n = 2.0, (<b>e</b>) n = 2.5, and (<b>f</b>) n = 3.0.</p>
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<p>Relationship curves of n and <math display="inline"><semantics> <mrow> <msub> <mrow> <mi>f</mi> </mrow> <mrow> <mi>Error</mi> <mfenced separators="|"> <mrow> <mi>n</mi> </mrow> </mfenced> </mrow> </msub> </mrow> </semantics></math> at different temperature intervals: (<b>a</b>) 900–950 °C and (<b>b</b>) 1000–1150 °C.</p>
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<p>Comparison of actual measured grain size and calculated value.</p>
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14 pages, 1339 KiB  
Article
Paraxial Propagation of Scattered Light Based on the Chirp Z-Transform
by Lujia Zhao, Yu-Ang Liu, Huiru Ji, Haibo Wang, Hao Tan, Yan Mo and Donglin Ma
Sensors 2025, 25(5), 1454; https://doi.org/10.3390/s25051454 - 27 Feb 2025
Viewed by 114
Abstract
In the simulation of partially coherent light propagation within optical systems utilizing the Wigner function, the constraints imposed by the Fourier transform necessitate that the dimensions of the input and output matrices remain congruent. Consequently, the extent of the image plane is dictated [...] Read more.
In the simulation of partially coherent light propagation within optical systems utilizing the Wigner function, the constraints imposed by the Fourier transform necessitate that the dimensions of the input and output matrices remain congruent. Consequently, the extent of the image plane is dictated by the dimensions of the light source matrix and the propagation distance. For optical systems of greater complexity, such simulations are highly memory-intensive. This paper innovatively incorporates the displacement theorem of the chirp z-transform and integrates it with the Wigner function. This approach affords enhanced flexibility in the simulation of partially coherent light transmission, enabling the targeted simulation of regions of interest within the frequency domain of the optical system, thereby significantly improving simulation efficiency. The efficacy of this novel method is demonstrated through the simulation of a Wigner transmission algorithm based on the chirp z-transform, applied to an RC (Ritchey–Chrétien) telescope system. The RC telescope, known for its optical design that minimizes aberrations and provides high-quality imaging, serves as a critical foundation for the simulation. The resultant simulations exhibit a high degree of consistency with traditional methods while offering increased flexibility, thus corroborating the validity and effectiveness of the proposed approach. Full article
(This article belongs to the Section Optical Sensors)
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Figure 1
<p>The profile of the RC telescope system.</p>
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<p>The profile of the optical surface error.</p>
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<p>The DFT-based Wigner distribution in the RC optical system: (<b>a</b>) Wigner distribution of the multi-Gauss Schell model beam; (<b>b</b>) Wigner distribution after free space propagation; (<b>c</b>) Wigner distribution HSF errors over the surface of the primary mirror; (<b>d</b>) Wigner distribution MSF errors over the surface of the primary mirror; (<b>e</b>) Wigner distribution of phase modulated by primary mirror; (<b>f</b>) free space transmission from primary mirror to secondary mirror; (<b>g</b>) Wigner distribution HSF errors over the surface of the secondary mirror; (<b>h</b>) Wigner distribution of phase modulated by primary mirror; (<b>i</b>) free space transmission from secondary mirror to the image plane.</p>
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<p>CZT-based Wigner distribution in the RC optical system: (<b>a</b>) Wigner distribution of the multi-Gauss Schell model beam; (<b>b</b>) Wigner distribution after free space propagation; (<b>c</b>) Wigner distribution HSF errors over the surface of the primary mirror; (<b>d</b>) Wigner distribution MSF errors over the surface of the primary mirror; (<b>e</b>) Wigner distribution of phase modulated by primary mirror; (<b>f</b>) free space transmission from primary mirror to secondary mirror; (<b>g</b>) Wigner distribution HSF errors over the surface of the secondary mirror; (<b>h</b>) Wigner distribution of phase modulated by primary mirror; (<b>i</b>) free space transmission from secondary mirror to the image plane.</p>
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<p>Light intensity distribution of RC telescope system: (<b>a</b>) DFT-based light intensity distribution; (<b>b</b>) CZT-based light intensity distribution.</p>
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<p>Comparison of light intensity between DFT and CZT methods on the detection plane.</p>
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