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Magnetic complexity of active regions during 23–24 solar cycles 23-24太阳周期活动区域的磁复杂性
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.1901
O. Baran, A. Prysiazhnyi, M. M. Koval'chuk
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引用次数: 2
Porous zinc oxide plate with micro- and nanoelements of the surface structure for heterogeneous photocatalysis 多孔氧化锌板具有微纳米元素的表面结构,用于多相光催化
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.3401
L. Hrytsak, B. Turko, V. Vasil’yev, R. Serkiz, A. Kostruba
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引用次数: 0
Influence of defects on adsorption processes in the near-surface layers of ZnO nanoclusters: MD study 缺陷对ZnO纳米团簇近表层吸附过程的影响:MD研究
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.1601
S. Savka, I. Mohylyak, D. Popovych
{"title":"Influence of defects on adsorption processes in the near-surface layers of ZnO nanoclusters: MD study","authors":"S. Savka, I. Mohylyak, D. Popovych","doi":"10.30970/jps.26.1601","DOIUrl":"https://doi.org/10.30970/jps.26.1601","url":null,"abstract":"","PeriodicalId":43482,"journal":{"name":"Journal of Physical Studies","volume":"15 1","pages":""},"PeriodicalIF":0.5,"publicationDate":"2022-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"87595160","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 1
X-ray spectroscopic properties and electronic structure of Ca3Ga2Ge4O14 Ca3Ga2Ge4O14的x射线光谱性质和电子结构
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.4701
I. Shcherba, L. Kostyk, L. Bekenov, M. Rudko, D. Uskokovi'c, H. Noga, R. Bilyk, B. M. Yatcyk, V. Denys
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引用次数: 0
Influence of hydrostatic pressure on dynamic dielectric characteristics of rbhso4 静水压力对rbhso4动态介电特性的影响
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.2701
A. Vdovych, R. Levitskii, I. R. Zachek, A. Moina
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引用次数: 0
Low-temperature technology for obtaining transparent ITO films with high conductivity 获得高导电性透明ITO薄膜的低温技术
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.4402
B. Turko, V. Vasiliev, Y. Eliyashevskyy, М. Rudko, N. Shvets, A. Vaskiv, L. Hrytsak, V. Kapustianyk, А. Kostruba, S. Semak
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引用次数: 0
Comparative study of spectral lines with different Landé factors observed in sunspots 太阳黑子不同地形因子光谱线的比较研究
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.4902
V. Lozitsky, S. Osipov, M. Stodilka
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引用次数: 1
Method of integral equations in the theory of rotational white dwarfs 旋转白矮星理论中的积分方程方法
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.1902
M. Vavrukh, S. Smerechynskyi, D. Dzikovskyi
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引用次数: 0
Features of growing Si- and Si1-xGex-single-crystal films from solution-melt based on tin 锡基溶液熔体生长Si和si1 - xgex单晶薄膜的特点
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2022-01-01 DOI: 10.30970/jps.26.4601
A. Razzokov, A. Saidov, V. Girzhon, O. Smolyakov
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引用次数: 0
Advanced morphology of VIPERS galaxies 毒蛇星系的高级形态
IF 0.5 Q3 PHYSICS, MULTIDISCIPLINARY Pub Date : 2021-10-22 DOI: 10.30970/jps.26.2901
O. Gugnin, A. Tugay, N. Pulatova, L. Zadorozhna
We calculated morphological parameters for 70821 galaxies from VIPERS (spectroscopic galaxy survey performed on VIMOS spectroscope at VLT). These parameters includes Gini, M20, Concentration, Asymmetry and Smoothness. Results correlate with the distribution of these parameters for other simulated and observed samples. We also studied dependence of these parameters with Sersic power index of radial distribution of surface brightness of galaxy image. Our aim was to find a clear separation of VIPERS galaxies on elliptical and spiral. This is necessary for testing the method of Sersic index (ns) calculation in statmorph program. To find such bimodality we use B-V color index from VIPERS database. To perform the error analysis of morphological parameters we simulated galaxy images with random background of different magnitude and estimated the errors as dispersion of the parameters. We also found asymptotic values of errors of morphological parameters by increasing the numbers of mock images. To analyse the possible variation of each morphological parameter during the convolution of close galactic images, we have simulated them to research. In the result of this investigation we have analysed the dependence of the every morphological parameter from CAS and Gini/M20 statistics from the distance between galactic centers. The differences between our results for VIPERS and Gini-M20 distribution for PanStarrs galaxies at z<0.5 could be explained it by cosmological evolution of galaxies. We found out that in modern Universe there are much more elliptical galaxies than at z>0.5 which corresponds to VIPERS sample. Also we concluded that galaxy mergers were more frequent in the early Universe.
我们计算了70821个星系的形态参数,这些星系是用VLT的VIMOS光谱仪进行的光谱星系调查。这些参数包括基尼系数、M20、浓度、不对称性和平滑度。结果与其他模拟和观测样本的这些参数分布相关联。我们还研究了这些参数与星系图像表面亮度径向分布的Sersic功率指数的相关性。我们的目标是在椭圆星系和螺旋星系上找到清晰的分离。这是测试statmorph程序中Sersic索引(ns)计算方法所必需的。为了找到这种双峰,我们使用了VIPERS数据库中的B-V颜色索引。为了对形态学参数进行误差分析,我们模拟了不同星等随机背景下的星系图像,并将误差估计为参数的色散。通过增加模拟图像的数量,我们也发现了形态学参数误差的渐近值。为了分析近距离星系图像在卷积过程中各形态参数可能发生的变化,我们对它们进行了模拟研究。在这项研究的结果中,我们分析了来自CAS和Gini/M20统计的每个形态学参数与星系中心之间距离的依赖关系。我们对VIPERS的结果与PanStarrs星系的Gini-M20分布在z0.5处的差异,对应于VIPERS样本。我们还得出结论,星系合并在早期宇宙中更为频繁。
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引用次数: 0
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Journal of Physical Studies
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