Journal of Quantitative Spectroscopy & Radiative Transfer最新文献_第3页

Contributions of argon, nitrogen, and oxygen to air broadening in the oxygen A-band 氩、氮和氧对氧a波段空气展宽的贡献

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-16 DOI: 10.1016/j.jqsrt.2025.109480

Leah E. Stevenson , Joshua L. Laughner , Mitchio Okumura , Joseph T. Hodges , Erin M. Adkins

{"title":"Contributions of argon, nitrogen, and oxygen to air broadening in the oxygen A-band","authors":"Leah E. Stevenson , Joshua L. Laughner , Mitchio Okumura , Joseph T. Hodges , Erin M. Adkins","doi":"10.1016/j.jqsrt.2025.109480","DOIUrl":"10.1016/j.jqsrt.2025.109480","url":null,"abstract":"<div><div>The oxygen (O<sub>2</sub>) A-band is used to determine the airmass in ground- and space-based remote sensing measurements because O<sub>2</sub> is well-mixed in the Earth’s atmosphere and its column-integrated amount fraction on a dry-gas basis is nearly constant. Because biases in the retrieved airmass propagate to measurements of target species, low-uncertainty spectroscopic parameters are essential for increasingly precise and accurate greenhouse gas measurements. However, laboratory measurements and atmospheric retrievals of this O<sub>2</sub> band typically neglect the line-shape effects caused by collisions with argon (Ar), which comprises 0.934 % by volume of the Earth’s atmosphere. To quantify the contribution of Ar to O<sub>2</sub> A-band air-broadening line-shape parameters, we measured pressure broadening and shifting parameters for ten high <em>J</em> lines in the P-branch of this band. These data were acquired in the laboratory over a range of pressures and nitrogen (N<sub>2</sub>), O<sub>2</sub>, and Ar amount fractions using cavity ring-down spectroscopy. Respective line-shape parameters for these collisional partners were determined with a multi-spectrum fitting algorithm. These results were combined with literature data to provide an empirical model for the rotational dependencies of the broadening and shifting parameters by each collisional partner. Incorporating these results into analyses of atmospheric column-integrated solar absorption spectra in the O<sub>2</sub> A-band shows that the neglect of Ar can lead to a small but potentially relevant systematic bias in surface pressure retrievals and a slight increase in the fit residuals of atmospheric spectra.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"342 ","pages":"Article 109480"},"PeriodicalIF":2.3,"publicationDate":"2025-04-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143873949","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Computation of K-shell X-ray Fluorescence Cross Section for photons ranging from 5.46keV to 123.6keV using three-dimensional semi-empirical formulae 用三维半经验公式计算5.46 ~ 123.6keV光子k壳层x射线荧光截面

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-16 DOI: 10.1016/j.jqsrt.2025.109479

K. Amari , A. Kahoul , J.M. Sampaio , S. Daoudi , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , Y. Kasri , A. Zidi , B. Berkani

{"title":"Computation of K-shell X-ray Fluorescence Cross Section for photons ranging from 5.46keV to 123.6keV using three-dimensional semi-empirical formulae","authors":"K. Amari , A. Kahoul , J.M. Sampaio , S. Daoudi , J.P. Marques , F. Parente , A. Hamidani , S. Croft , A. Favalli , Y. Kasri , A. Zidi , B. Berkani","doi":"10.1016/j.jqsrt.2025.109479","DOIUrl":"10.1016/j.jqsrt.2025.109479","url":null,"abstract":"<div><div>In this work, we propose a novel three-dimensional semi-empirical formula for the estimation of K-shell X-ray fluorescence cross sections for a wide range of elements <span><math><mrow><mn>16</mn><mo>≤</mo><mi>Z</mi><mo>≤</mo><mn>92</mn></mrow></math></span> based on the database of the experimental values published between 1985 and 2023 for photons spanning from 5.46 to 123.6 keV (over 3300 data). This approach employs an analytical dependent on the atomic number Z and the energy E. Subsequently, the ratio <span><math><mrow><msub><mi>S</mi><mi>W</mi></msub><mo>=</mo><mrow><mo>(</mo><msub><mi>σ</mi><mrow><mi>K</mi><mi>i</mi><mo>−</mo><mi>E</mi><mi>x</mi><mi>p</mi></mrow></msub><mo>)</mo></mrow><mo>/</mo><mrow><mo>(</mo><msub><mi>σ</mi><mrow><mi>K</mi><mi>i</mi><mo>−</mo><mi>W</mi></mrow></msub><mo>)</mo></mrow></mrow></math></span> are fitted using a three-dimension polynomial function, in terms of the atomic number Z and energy E. The cross-sections were described as the product of two functions, the first is a polynomial that represents the weighted mean of cross-sections values across different conditions and the second function provides additional fitting to the cross-section based on atomic numbers Z and energy E. The cross-sections expressed as function of these two variables show reasonable agreement with the experimental values.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"342 ","pages":"Article 109479"},"PeriodicalIF":2.3,"publicationDate":"2025-04-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143863349","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Surface-integral-equation solution for solid particles with wavelength-scale surface roughness 具有波长尺度表面粗糙度的固体颗粒的表面积分方程解决方案

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-12 DOI: 10.1016/j.jqsrt.2025.109467

Johannes Markkanen

{"title":"Surface-integral-equation solution for solid particles with wavelength-scale surface roughness","authors":"Johannes Markkanen","doi":"10.1016/j.jqsrt.2025.109467","DOIUrl":"10.1016/j.jqsrt.2025.109467","url":null,"abstract":"<div><div>A Surface Integral Equation (SIE) method has been implemented to analyze light scattering by arbitrarily shaped solid dielectric particles. Specifically, the Poggio–Miller–Chang–Harrington–Wu–Tsai formulation is discretized using the Galerkin method, employing Rao–Wilton–Glisson basis functions. The numerical solution is further accelerated through the application of the high-frequency Multilevel Fast Multipole Algorithm (MLFMA). This MLFMA-accelerated SIE solution demonstrates efficiency for homogeneous particles with moderately rough surfaces, even in the absence of advanced preconditioning techniques and broadband MLFMA. Notably, as the number of unknowns scales with the surface area, the SIE solution offers a distinct advantage over traditional volumetric methods, such as the discrete-dipole approximation and finite-element methods, where the number of unknowns scales with the volume of the scatterer. The SIE method is employed to investigate light scattering by homogeneous particles with rough surfaces, and the results are compared to the geometric optics approximation. It is demonstrated that the geometric optics approximation yields poor accuracy for particles with self-affine surface roughness.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"341 ","pages":"Article 109467"},"PeriodicalIF":2.3,"publicationDate":"2025-04-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143832559","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Effect of charged sand grains in strong sandstorms on microwave radar range 强沙尘暴中带电沙粒对微波雷达距离的影响

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-09 DOI: 10.1016/j.jqsrt.2025.109468

Qiang Ma, Yue Xi, Li Xie

{"title":"Effect of charged sand grains in strong sandstorms on microwave radar range","authors":"Qiang Ma, Yue Xi, Li Xie","doi":"10.1016/j.jqsrt.2025.109468","DOIUrl":"10.1016/j.jqsrt.2025.109468","url":null,"abstract":"<div><div>In this paper, the range of low-frequency microwave radar going through sand storms is numerically investigated with considering the attenuation and backscattering of charged sand grains along the link. It was found that strong sandstorms can reduce the range of microwave radar, which is reduced by < 5 % for radars at the L and S bands when the visibility is larger than 50 m; while with the visibility of 10 m, the radar range at the L(1.215G Hz), S(3 GHz), and X(10 GHz) bands is reduced by 27.69 %, 31.90 % and 89.69 %. The charges carried by sand grains increase the reduction. Due to the scattering of radar waves by sand grains along the link, the signal-to-noise ratio (SNR) will decrease with the radar detection distance. Near the radar system, SNR decreases rapidly due to the strong attenuation of sand storms, which will cause a detection blind zone near the radar systems, which is related to the visibility, the RCS, and radar frequency. Charges carried on sand grains reduce the SNR to expand the blind zone in sandstorms. Given the target, it is necessary to increase the radar frequency or reduce the minimum detectable SNR of a radar system to avoid the detection blind zone near the radar.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"341 ","pages":"Article 109468"},"PeriodicalIF":2.3,"publicationDate":"2025-04-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143839028","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Line strength analysis of the 12CD4 infrared spectra in the pentad region 五边形区域12CD4红外光谱的线强度分析

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-07 DOI: 10.1016/j.jqsrt.2025.109453

O.N. Ulenikov , O.V. Gromova , E.S. Bekhtereva , N.I. Nikolaeva , X. Guan , C. Sydow , S. Bauerecker

{"title":"Line strength analysis of the 12CD4 infrared spectra in the pentad region","authors":"O.N. Ulenikov , O.V. Gromova , E.S. Bekhtereva , N.I. Nikolaeva , X. Guan , C. Sydow , S. Bauerecker","doi":"10.1016/j.jqsrt.2025.109453","DOIUrl":"10.1016/j.jqsrt.2025.109453","url":null,"abstract":"<div><div>High accurate ro-vibrational spectra of <span><math><msup><mrow></mrow><mrow><mn>12</mn></mrow></msup></math></span>CD<span><math><msub><mrow></mrow><mrow><mn>4</mn></mrow></msub></math></span> were measured in the pentad region with a Bruker IFS125 HR Fourier transform infrared (IR) spectrometer at an optical resolution of 0.003 cm<sup>−1</sup> and different pressures and optical path-lengths. The analysis of 1264 experimental absolute transition strengths belonging to all nine ro-vibrational sub-bands of the <span><math><msup><mrow></mrow><mrow><mn>12</mn></mrow></msup></math></span>CD<span><math><msub><mrow></mrow><mrow><mn>4</mn></mrow></msub></math></span> pentad was performed using the Voigt profile to simulate the measured line shape and to determine experimental line intensities. A set of 10 parameters was obtained from the weighted fit analysis of experimental data in the frame of the model of an effective dipole moment operator of the <span><math><msup><mrow></mrow><mrow><mn>12</mn></mrow></msup></math></span>CD<span><math><msub><mrow></mrow><mrow><mn>4</mn></mrow></msub></math></span> pentad. The obtained set of 10 effective dipole moment parameters reproduces the initial 1264 absolute transition strengths with the d<span><math><mrow><msub><mrow></mrow><mrow><mtext>rms</mtext></mrow></msub><mo>=</mo><mn>4</mn><mo>.</mo><mn>52</mn><mtext>%</mtext></mrow></math></span>. A line list of the studied experimental ro-vibrational transitions up to <span><math><mrow><mi>J</mi><mo>≤</mo><mn>25</mn></mrow></math></span> is presented in the Supplementary data to this paper.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"341 ","pages":"Article 109453"},"PeriodicalIF":2.3,"publicationDate":"2025-04-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143799759","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

Erratum: Absorption cross sections of n-butane, n-pentane, cyclopentane and cyclohexane 勘误：正丁烷、正戊烷、环戊烷和环己烷的吸收截面

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-05 DOI: 10.1016/j.jqsrt.2025.109455

Jason J. Sorensen , Peter F. Bernath , Ryan M. Johnson , Randika Dodangodage , W. Doug Cameron , Keith LaBelle

引用次数: 0

Preface electromagnetic and light scattering XX. Topical issue 电磁与光散射XX。局部问题

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-05 DOI: 10.1016/j.jqsrt.2025.109465

Olga Muñoz, Elisa Frattin, Julia Martikainen

引用次数: 0

Near- and mid-infrared spectroscopy of isobutyronitrile and cyanopropyne: absorption cross-sections for quantitative detection in astrophysical objects 异丁腈和氰基丙炔的近红外和中红外光谱：用于天体物理天体定量探测的吸收截面

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-04 DOI: 10.1016/j.jqsrt.2025.109466

D. Jacquemart , B. Tremblay , P. Soulard , L. Krim , J.C. Guillemin , A. Coustenis , T. Encrenaz , P. Lavvas , T.K. Greathouse , R. Giles

{"title":"Near- and mid-infrared spectroscopy of isobutyronitrile and cyanopropyne: absorption cross-sections for quantitative detection in astrophysical objects","authors":"D. Jacquemart , B. Tremblay , P. Soulard , L. Krim , J.C. Guillemin , A. Coustenis , T. Encrenaz , P. Lavvas , T.K. Greathouse , R. Giles","doi":"10.1016/j.jqsrt.2025.109466","DOIUrl":"10.1016/j.jqsrt.2025.109466","url":null,"abstract":"<div><div>Absorption cross-sections at room temperature have been derived for two non-cyclic organic molecules cyanopropyne (CH<sub>3</sub>C<sub>3</sub>N) and isobutyronitrile (i-C<sub>3</sub>H<sub>7</sub>CN), and have been proposed for the 2024 update of the <em>hi</em>gh-resolution <em>tran</em>smission molecular absorption database (HITRAN). The gas phase infrared spectra of pure cyanopropyne and isobutyronitrile have been recorded at room temperature between 160 and 3500 cm<sup>-1</sup> (3–60 µm) using an infrared Fourier transform spectrometer. The spectral resolution has been chosen equal to 0.056 cm<sup>-1</sup>. For the 18–20 µm spectral region an additional resolution equal to 0.01 cm<sup>-1</sup> has been used. Among the various absorption bands observed, some of them, as the ν<sub>10</sub> band of cyanopropyne around 500 cm<sup>-1</sup> (20 µm), are particularly interesting for detecting and quantifying these molecules in astrophysical objects. As a first application, the retrieved absorption cross-sections have been used in a radiative transfer code to simulate observations of Titan's stratosphere acquired using the Texas Echelon Cross Echelle Spectrograph (TEXES at the Infrared Telescope Facility (IRTF, Mauna Kea Observatory). We discuss preliminary results and perspectives, among which estimated upper limits of 3 × 10<sup>–9</sup> for cyanopropyne and 3 × 10<sup>–7</sup> for isobutyronitrile in Titan's stratosphere.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"341 ","pages":"Article 109466"},"PeriodicalIF":2.3,"publicationDate":"2025-04-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143817756","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

New relationships relating acoustical and electromagnetic beam shape coefficients 声学和电磁波束形状系数的新关系

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-03 DOI: 10.1016/j.jqsrt.2025.109451

Gérard Gouesbet , Jianqi Shen , Leonardo A. Ambrosio

{"title":"New relationships relating acoustical and electromagnetic beam shape coefficients","authors":"Gérard Gouesbet , Jianqi Shen , Leonardo A. Ambrosio","doi":"10.1016/j.jqsrt.2025.109451","DOIUrl":"10.1016/j.jqsrt.2025.109451","url":null,"abstract":"<div><div>It has been recently demonstrated that the electromagnetic beam shape coefficients <span><math><msubsup><mrow><mi>g</mi></mrow><mrow><mi>n</mi><mo>,</mo><mi>X</mi></mrow><mrow><mi>m</mi></mrow></msubsup></math></span> (<span><math><mrow><mi>X</mi><mo>=</mo><mi>T</mi><mi>M</mi></mrow></math></span> or <span><math><mrow><mi>T</mi><mi>E</mi></mrow></math></span>) which encode the structure of structured light beams may be expressed in terms of scalar, more specifically acoustical, beam shape coefficients. Because the technique used to obtain the relevant expressions relied on the properties of what is known as the finite series method, the aforementioned expressions were different, depending on whether <span><math><mrow><mo>(</mo><mi>n</mi><mo>−</mo><mi>m</mi><mo>)</mo></mrow></math></span> is even or odd. For a reason discussed in the bulk of the paper, it became obvious that the expressions obtained for different parities of <span><math><mrow><mo>(</mo><mi>n</mi><mo>−</mo><mi>m</mi><mo>)</mo></mrow></math></span> could be unified. Proceeding to such an unification, the expressions previously published were not only unified, but furthermore simplified, then allowing for an easier and less time-consuming numerical implementation.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"340 ","pages":"Article 109451"},"PeriodicalIF":2.3,"publicationDate":"2025-04-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143768012","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0

MARVEL analysis of high-resolution rovibrational spectra of 16O12C17O 16O12C17O高分辨率旋转振动光谱的MARVEL分析

IF 2.3 3区物理与天体物理

Journal of Quantitative Spectroscopy & Radiative Transfer Pub Date : 2025-04-01 DOI: 10.1016/j.jqsrt.2025.109444

Saja A.M. Obaidat , Ala’a A.A. Azzam , Dunia Alatoom , Mohammad Taha I. Ibrahim , Jonathan Tennyson , Tibor Furtenbacher , Attila G. Császár

{"title":"MARVEL analysis of high-resolution rovibrational spectra of 16O12C17O","authors":"Saja A.M. Obaidat , Ala’a A.A. Azzam , Dunia Alatoom , Mohammad Taha I. Ibrahim , Jonathan Tennyson , Tibor Furtenbacher , Attila G. Császár","doi":"10.1016/j.jqsrt.2025.109444","DOIUrl":"10.1016/j.jqsrt.2025.109444","url":null,"abstract":"<div><div><sup>16</sup>O<sup>12</sup>C<sup>17</sup>O is the fourth most abundant isotopologue of carbon dioxide. As part of this study, a total of 16223 rovibrational transitions, 9822 unique ones, measured for the ground electronic state of CO<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span>, were collected from 31 articles, corresponding to the limited wavenumber range of 634–12727 cm<sup>−1</sup>. The measured transitions span the polyads <span><math><mrow><mi>P</mi><mo>=</mo><mn>0</mn><mo>−</mo><mn>17</mn></mrow></math></span>, where <span><math><mrow><mi>P</mi><mo>=</mo><mn>2</mn><msub><mrow><mi>v</mi></mrow><mrow><mn>1</mn></mrow></msub><mo>+</mo><msub><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow></msub><mo>+</mo><mn>3</mn><msub><mrow><mi>v</mi></mrow><mrow><mn>3</mn></mrow></msub></mrow></math></span>, and <span><math><msub><mrow><mi>v</mi></mrow><mrow><mn>1</mn></mrow></msub></math></span>, <span><math><msub><mrow><mi>v</mi></mrow><mrow><mn>2</mn></mrow></msub></math></span>, and <span><math><msub><mrow><mi>v</mi></mrow><mrow><mn>3</mn></mrow></msub></math></span> are the normal-mode quantum numbers corresponding to the symmetric stretch, linear bend, and antisymmetric stretch motions. Following a careful validation of the compiled rovibrational transitions data, a set of 5036 empirical rovibrational energy levels has been determined. Comparison of the empirical energy-level data of this study with those in the CDSD-296 and NASA Ames-2021 line lists shows good general agreement.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"340 ","pages":"Article 109444"},"PeriodicalIF":2.3,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143768013","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}

引用次数: 0