Radio SciencePub Date : 2025-04-01DOI: 10.1029/2024RS008142
Ahmet Uluslu;Kervendurdy Allaberdiyev
{"title":"Competitive metaheuristic algorithms for building a performance database of a dual-band combline bandpass filter with microstrip connection","authors":"Ahmet Uluslu;Kervendurdy Allaberdiyev","doi":"10.1029/2024RS008142","DOIUrl":"https://doi.org/10.1029/2024RS008142","url":null,"abstract":"Dual-band bandpass filters have attracted intense attention in recent developments to meet many demands, especially wireless applications and multi-band radio wave. Here, a Combline filter in the form of a dual bandpass 3-row microstrip with a center resonance frequency of 2.5 and 3.0 GHz and a total of 13 design parameters, 6 of which are variable, has become a single-objective and multi-dimensional optimization design problem with the help of current competitive metaheuristic algorithms. Algorithms have been derived in recent years, have proven their success against existing algorithms, and have not been used in the filter design problem. In addition, in a different study conducted in recent years, among five different objective function pairs that were fabricated from mathematical models that have proven successful, the three most successful objective function pairs were selected based on the relevant study results and these objective function pairs were adapted for the filter and included in the study. Throughout this design optimization process, the filter toolbox in the R2023B version, available as of the MATLAB R2022B version, was used. In addition to the original objective function, the study includes multiple innovations such as the new filter toolbox and current competitive metaheuristic algorithms. During this entire optimization process, the most optimal results are verified by electromagnetic simulation. Considering all these results in the study, the optimization processes performed with the proposed competitive algorithms are an easy, fast and efficient solution for complex and multi-dimensional filter design optimization applications. Additionally, it can be quickly applied to other microwave optimization problems by changing the objective functions.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 4","pages":"1-18"},"PeriodicalIF":1.6,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143908345","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-04-01DOI: 10.1029/2025RS008270
Kazuya Kobayashi;Jothiram Vivekanandan
{"title":"Thank you to our 2024 reviewers","authors":"Kazuya Kobayashi;Jothiram Vivekanandan","doi":"10.1029/2025RS008270","DOIUrl":"https://doi.org/10.1029/2025RS008270","url":null,"abstract":"The Editors thank the 2024 peer reviewers. As you are aware, the journal Radio Science (RDS) publishes original research papers on electromagnetic propagation and its applications. In 2024, we received a total of 206 manuscripts for consideration for publication in the RDS. We tried very carefully to find reviewers who were best fit to the topics of manuscripts. You worked hard in the peer-review process and gave us excellent evaluations. Our journal would never have kept a high reputation without your continued efforts. Thank you all for your significant contributions to the review process and we look forward to working with you also this year and in the coming years.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 4","pages":"1-4"},"PeriodicalIF":1.6,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143908348","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-04-01DOI: 10.1029/2024RS008157
P. Chowdhury;E. Spencer;P. Adhya;S. Patra;S. K. Vadepu;P. S. Rayapati
{"title":"Analysis of sweeping impedance probe measurements in the F-layer of the ionosphere during the occurrence of a mid-latitude spread F event","authors":"P. Chowdhury;E. Spencer;P. Adhya;S. Patra;S. K. Vadepu;P. S. Rayapati","doi":"10.1029/2024RS008157","DOIUrl":"https://doi.org/10.1029/2024RS008157","url":null,"abstract":"Plasma Impedance Probes (PIP) are AC instruments that are used to measure and observe resonances and damping features in plasmas. These probes are typically flown on sounding rocket missions studying ionosphere plasma physics. In this work we present a combined circuit—empirical model for the frequency dependent impedance of a monopole probe on a sounding rocket payload that traverses multiple ionospheric layers. The purpose of this model is to resolve some difficulties encountered when interpreting and analyzing PIP measurements made at the higher altitudes during the Tropical STORMS sounding rocket launched from Wallops Island, Virginia, in 2007. In an earlier work (Spencer & Patra, 2015, https://doi.org/10.1002/2015rs005697), we identified the presence of anomalous damping in the measurements above 260 km. Here, we introduce a more detailed model of the plasma probe interaction to explain these observations. The new model incorporates the effect of a sheath, and some additional parallel conductivity elements that dampen the observed impedance in the F-layer of the ionosphere. We show that by accounting for the presence and gradual impact of the parallel conductance elements, the PIP data can be accurately analyzed and interpreted. We hypothesize that secondary electrons with higher mobilities may contribute to the observed effects, and propose future investigations that may be conducted to further understand the observations.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 4","pages":"1-19"},"PeriodicalIF":1.6,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143908279","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-04-01DOI: 10.1029/2025RS008217
Hanene Zormati;Jalel Chebil;Jamel Bel Hadj Tahar
{"title":"Impact of static and mobile scatterers on vehicle-to-vehicle communication channel in rectangular tunnel environment","authors":"Hanene Zormati;Jalel Chebil;Jamel Bel Hadj Tahar","doi":"10.1029/2025RS008217","DOIUrl":"https://doi.org/10.1029/2025RS008217","url":null,"abstract":"Vehicle-to-Vehicle communication has received a lot of attention over recent years since it can improve the efficiency and safety of roads. One of the research area in this topic is channel modeling. In this paper, a three-dimensional wideband regular shaped geometry based channel model for multiple-input and multiple-output vehicle-to-vehicle communication channel is proposed for rectangular tunnel environments. A two cylindrical geometry is adopted to describe moving vehicles around transmitter and receiver, and a cuboid model is employed to depict scatterers located on internal surfaces of the tunnel walls. Using this channel model, the channel characteristics including space time correlation function, frequency correlation function, autocorrelation function, power spectral density and channel capacity are derived and simulated numerically. Finally, the impact of channel parameters on the performance of the channel model is analyzed. Results confirm the efficiency of the proposed model in comparison with other models.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 4","pages":"1-10"},"PeriodicalIF":1.6,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143908346","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-04-01DOI: 10.1029/2025RS008218
Faiz ur Rehman;Zicheng Liu;Miao Cao;Yali Zong
{"title":"Design of a simple and efficient ultra-wideband dipole-structured cross-polarization conversion metasurface","authors":"Faiz ur Rehman;Zicheng Liu;Miao Cao;Yali Zong","doi":"10.1029/2025RS008218","DOIUrl":"https://doi.org/10.1029/2025RS008218","url":null,"abstract":"Electromagnetic applications frequently necessitate precise polarization control, such as converting horizontal polarization to vertical. This work introduces an innovative reflection mode metasurface that rotates the state of linearly polarized electromagnetic waves in the microwave spectrum. The envisioned unit cell has three layers that make up its symmetry: a reflective copper surface at the bottom, a 3 mm thick F4BM substrate in the center, and a copper patch having tiny strips on both sides and a 45° angled dipole structure on top. With a fractional bandwidth of 98%, this unit cell can rotate components of linear polarized signals by 90° in the ultra-wideband frequency range (8.6∼25.3 GHz). In the required frequency spectrum, the surface has excellent polarization conversion ability, which is calculated as the polarization conversion ratio (PCR), which is nearly equal to 95%. The surface also shows stability to oblique angle incidence in the wide band. The suggested metasurface has significant uses in antenna design, wireless communication, and stealth technology.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 4","pages":"1-12"},"PeriodicalIF":1.6,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143908347","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-04-01DOI: 10.1029/2024RS008103
Y. Liu;M. Füllekrug
{"title":"Correlation between the delay and rise time of VLF/LF amplitudes during 20 solar X-ray flares observed in February 2014 at mid-latitude","authors":"Y. Liu;M. Füllekrug","doi":"10.1029/2024RS008103","DOIUrl":"https://doi.org/10.1029/2024RS008103","url":null,"abstract":"During daylight hours, the concentration of electrons in the ionosphere can be amplified by solar flares, which may subsequently influence the propagation of radio waves. Previous research on Very Low Frequency (VLF) signals focused on X-class and M-class flares. This study expands the scope to include a broader frequency range and C-class flares. During 20-28 February 2014, signals from 15 transmitters (18.3—81.0 kHz) were recorded by a receiver in Bath, UK. 20 solar flares captured during this period are investigated. A new methodology was employed to determine the rise times of the received amplitudes for comparison with the solar X-ray flux recorded by the Geostationary Operational Environmental Satellite geostationary satellite. The time delays between the onset of the X-ray flux and the onset of received amplitude changes are calculated. The general trend shows that shorter delays are linearly correlated to longer rise times of the amplitudes. It is found that the absolute slopes of the linear correlation between the delay and the rise time of M-class flares are larger than those of C-class flares. Two flares showed onset times of received amplitudes preceding the X-ray flux onset. A possible explanation for this is that the received signals might also be influenced by hard X-rays rather than the analyzed soft X-rays. In summary, this study demonstrates the effects of small C-class and M- class flares on the propagation of VLF/LF signals and offers insights for further research on solar flare impacts on radio waves and the lower ionosphere.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 4","pages":"1-16"},"PeriodicalIF":1.6,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143908358","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-04-01DOI: 10.1029/2024RS008197
Xun Wang;Yunhua Zhang;Dong Li
{"title":"Complex polarizations of ionospheric characteristic waves: A revisit in terms of real representation","authors":"Xun Wang;Yunhua Zhang;Dong Li","doi":"10.1029/2024RS008197","DOIUrl":"https://doi.org/10.1029/2024RS008197","url":null,"abstract":"The polarizations of ionospheric characteristic waves (CWs) are determined by the two solutions of the quadratic equation in the complex polarization ratio R within the magneto-ionic theory. This paper revisits these solutions and their relationship from the perspective of real representation, given that various real polarization parameter sets are also commonly used and play important parts in characterizing wave polarization. Multiple two-dimensional (2D) real representations are analyzed by re-examining several real two- parameter sets mathematically under a unified framework to prevent possible confusion from examining different parameters in separate frameworks, and by graphically representing the polarizations of the two CWs using 2D polarization plane plots constructed from paired real parameters. A three-dimensional (3D) real representation as the extension of two dimensions is further considered by the mathematical re-examination of the three normalized Stokes parameters for the two CWs and the application of the 3D Poincaré sphere visualization to overcome the non-uniform polarization distribution on the plane plot and the non-unique correspondence between plane point and polarization state. Each real parameter in these real representations is expressed as a function of R. Importantly, the relationship between the same real parameters of the two CWs is derived. Numerical examples presented through the polarization plane or Poincaré sphere plot demonstrate how these real parameters vary with certain ionosphere medium-related quantities and validate the correctness of the derived relationships. The comparison of each real representation with and without collisions reveals the impact of collisions on the real parameters and polarization orthogonality of the two CWs.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 4","pages":"1-27"},"PeriodicalIF":1.6,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143908337","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-03-01DOI: 10.1029/2024RS008150
P. Teysseyre;C. Briand;R. Marshall;M. Cohen
{"title":"Effect of ground conductivity on VLF wave propagation","authors":"P. Teysseyre;C. Briand;R. Marshall;M. Cohen","doi":"10.1029/2024RS008150","DOIUrl":"https://doi.org/10.1029/2024RS008150","url":null,"abstract":"Very Low Frequency (VLF, 3–30 kHz) waves propagate long distances in the waveguide formed by the Earth and the lower ionosphere. External sources such as solar flares and lightning discharges perturb the upper waveguide boundary and thereby modify the waves propagating within it. Therefore, studying the propagation of VLF waves within the waveguide enables us to probe the ionospheric response to external forcing. However, the wave propagation also depends on the lower waveguide boundary property, that is, the path conductivity. We tackle two main questions: how accurate should the path conductivity description be to obtain a given accuracy on the ionospheric electron density? Are the currently available ground-conductivity maps accurate enough? The impact of the ground conductivity values and their spatial extension on VLF wave propagation is studied through modeling with the Longwave Mode Propagator code. First, we show that knowledge of the path conductivity value should be more accurate as the ground conductivity decreases, in particular in regions where σ ≤ 10<sup>−3</sup> S/m. Second, we find that wave propagation is strongly sensitive to the spatial extension of ground conductivity path segments: segments of a few tens of km should be included in the path description to maintain below 50% the error on the derived electron density due to the path description. These results highlight the need for an update of the ground conductivity maps, to get better spatial resolution, more accurate values, and an estimate of the time-variability of each region.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 3","pages":"1-16"},"PeriodicalIF":1.6,"publicationDate":"2025-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143769445","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Radio SciencePub Date : 2025-03-01DOI: 10.1029/2024RS008112
Liu Yu;Du Yongxing;Li Baoshan;Qin Ling;Li Chenlu
{"title":"Fractional OAM vortex SAR imaging based on chirp scaling algorithm","authors":"Liu Yu;Du Yongxing;Li Baoshan;Qin Ling;Li Chenlu","doi":"10.1029/2024RS008112","DOIUrl":"https://doi.org/10.1029/2024RS008112","url":null,"abstract":"Vortex electromagnetic wave carries orbital angular momentum. Combined with Doppler information provided by radar platform movement, vortex electromagnetic wave can achieve higher resolution target imaging in SAR Imaging technology. In this paper, fractional order OAM vortex SAR imaging is studied. Firstly, the side-looking strip SAR imaging model is established. Then, the scattering echo equation of fractional order OAM is derived. Finally, the imaging simulation of multi-point target and single point target under Gaussian SNR is carried out by Chirp Scaling algorithm. The experimental results show that compared with the integer order OAM Vortex SAR Imaging, the fractional order OAM Vortex SAR Imaging in this paper has stronger robustness in Multi-target and Noise environment, which proves the effectiveness of the fractional order Vortex SAR Imaging.","PeriodicalId":49638,"journal":{"name":"Radio Science","volume":"60 3","pages":"1-14"},"PeriodicalIF":1.6,"publicationDate":"2025-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143769444","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}