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Chinese Academy of Sciences Institutional Repositories Grid
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CAS IR Grid
机构
金属研究所 [9]
福建物质结构研究所 [6]
国家天文台 [4]
地质与地球物理研究所 [3]
国家空间科学中心 [3]
合肥物质科学研究院 [3]
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OAI收割 [44]
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期刊论文 [43]
会议论文 [1]
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2024 [1]
2023 [2]
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Effects of vacuum magnetic field region on the compact torus trajectory in a tokamak plasma
期刊论文
OAI收割
PLASMA SCIENCE & TECHNOLOGY, 2024, 卷号: 26
作者:
Dong, Qilong
;
Zhang, Jie
;
Lan, Tao
;
Xiao, Chijin
;
Zhuang, Ge
  |  
收藏
  |  
浏览/下载:10/0
  |  
提交时间:2024/11/22
compact torus
central fueling
vacuum magnetic field region
penetration mechanism
optimization parameters
Recovering the Near-Surface Magnetic Image of Mercury from Satellite Observations
期刊论文
OAI收割
REMOTE SENSING, 2023, 卷号: 15, 期号: 8, 页码: 15
作者:
Kolotov, Igor
;
Lukyanenko, Dmitry
;
Stepanova, Inna
;
Wang, Yanfei
;
Yagola, Anatoly
  |  
收藏
  |  
浏览/下载:16/0
  |  
提交时间:2023/12/29
magnetic parameters reconstruction
magnetic image
Mercury
MESSENGER
inverse problem
regularization
Photometric Properties and Stellar Parameters of the Rapidly Rotating Magnetic Early-B Star HD 345439
期刊论文
OAI收割
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2023, 卷号: 23, 期号: 1, 页码: 14
作者:
Shen, Dong-Xiang
;
Liu, Jin-Zhong
;
Zhu, Chun-Hua
;
Lu, Guo-Liang
;
Zhang, Yu
  |  
收藏
  |  
浏览/下载:48/0
  |  
提交时间:2023/03/01
stars: chemically peculiar
stars: early-type
stars: fundamental parameters
stars: magnetic field
On the Relation Between Coronal Green Line Brightness and Magnetic Fields Intensity
期刊论文
OAI收割
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2022, 卷号: 22, 期号: 7
作者:
Zhang XF(张雪飞)
;
Liu Y(刘煜)
;
Zhao MY(赵明宇)
;
Song TF(宋腾飞)
  |  
收藏
  |  
浏览/下载:42/0
  |  
提交时间:2022/06/27
Sun: magnetic fields
Sun: corona
Stars: coronae
Sun: activity
Sun: atmosphere
Sun: coronal mass ejections (CMEs)
Sun: fundamental parameters
Sun: heliosphere
Sun: UV radiation
The Analgesic Effects of Static Magnetic Fields
期刊论文
OAI收割
BIOELECTROMAGNETICS, 2021, 卷号: 42
作者:
Fan, Yixiang
;
Ji, Xinmiao
;
Zhang, Lei
;
Zhang, Xin
  |  
收藏
  |  
浏览/下载:38/0
  |  
提交时间:2021/03/15
magnetic fields (MFs)
negative effects
pain management
positive effects
SMF parameters
Magnetized Particle Motion around Black Holes in Conformal Gravity: Can Magnetic Interaction Mimic Spin of Black Holes?
期刊论文
OAI收割
UNIVERSE, 2020, 卷号: 6, 期号: 3, 页码: 20
作者:
Haydarov, Kamoliddin
;
Abdujabbarov, Ahmadjon
;
Rayimbaev, Javlon
;
Ahmedov, Bobomurat
  |  
收藏
  |  
浏览/下载:20/0
  |  
提交时间:2021/12/06
black hole
magnetized particle motion
magnetic field
conformal gravity
constraints on black hole parameters
From polarimetry to helicity: Studies of solar magnetic fields at the Huairou Solar Observing Station
期刊论文
OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2019, 卷号: 62, 期号: 9, 页码: 18
作者:
Zhang, HongQi
  |  
收藏
  |  
浏览/下载:49/0
  |  
提交时间:2020/03/10
solar spectrum
polarization-stokes parameters
magnetic fields-current and helicity
MAGNETIC PARAMETERS INVERSION METHOD WITH FULL TENSOR GRADIENT DATA
期刊论文
OAI收割
INVERSE PROBLEMS AND IMAGING, 2019, 卷号: 13, 期号: 4, 页码: 745-754
作者:
Wang, Yanfei
;
Lukyanenko, Dmitry
;
Yagola, Anatoly
  |  
收藏
  |  
浏览/下载:43/0
  |  
提交时间:2019/07/29
Full tensor magnetic gradient
magnetic parameters reconstruction
regularization
On the possibility of disk-fed formation in supergiant high-mass X-ray binaries
期刊论文
OAI收割
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2019, 卷号: 19, 期号: 1, 页码: 8
作者:
Taani, Ali
;
Karino, Shigeyuki
;
Song, Liming
;
Al-Wardat, Mashhoor
;
Khasawneh, Awni
  |  
收藏
  |  
浏览/下载:16/0
  |  
提交时间:2020/03/10
binaries: X-rays
stars: neutron
stars: fundamental parameters
accretion disks
formation
magnetic fields
A New Set of Parameters of High-Mass X-ray Binaries Found with their Cyclotron Lines
期刊论文
OAI收割
arXiv e-prints, 2018
作者:
Zhang, Chengmin
;
Taani, Ali
;
Chaty, Sylvain
;
Karino, Shigeyuki
;
Song, Liming
  |  
收藏
  |  
浏览/下载:77/0
  |  
提交时间:2019/07/12
Astrophysics - High Energy Astrophysical Phenomena
Abstract: We have derived new physical quantities for several High-Mass X-ray Binaries (HMXBs) with supergiant (SG) companions through their cyclotron lines. The parameters are: the terminal velocity of the wind, the mass loss rate of the donor, the effective temperature and the magnetic fields. These parameters influence significantly the improvement of the model of accretion. In spite of the variety of their observational properties, the corresponding magnetic field is around B ~ 10^12 G. This result can be constrained by the effects on stellar evolution. In addition, we have performed a segmentation in the parameter space of donors intended for several SG-HMXB listed in our sample set. The parameter space can be categorized into five regimes depending on the possibility of disk formation associated with accretion from the stellar wind. This can give a quantitative clarification of the observed variability and the properties of these objects. We show that, when these systems come into the direct accretion region, systems with corresponding parameters can emit X-rays.