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查看斯高帕斯 (Scopus) 概要
陳 文屏
教授
天文研究所
https://orcid.org/0000-0003-0262-272X
電子郵件
wchen
astro.ncu.edu
tw
網站
http://www.astro.ncu.edu.tw/people/faculty_bio.php?id=4
h-index
9852
引文
54
h-指數
按照存儲在普爾（Pure）的出版物數量及斯高帕斯（Scopus）引文計算。
1990 …
2025
每年研究成果
概覽
指紋
網路
研究計畫
(15)
研究成果
(311)
資料集
(49)
類似的個人檔案
(6)
指紋
查看啟用 Wen-Ping Chen 的研究主題。這些主題標籤來自此人的作品。共同形成了獨特的指紋。
排序方式
重量
按字母排序
Keyphrases
Blazars
82%
Light Curves
78%
Occultations
65%
Star Formation
62%
X-ray
60%
Open Clusters
53%
Star Forming Regions
48%
Magnetic Field
47%
Radio
42%
Photometry
40%
Spectral Energy Distribution
36%
Near-infrared
36%
Swift
35%
Synchrotron
35%
Galactic
33%
High Energy
32%
Molecular Clouds
31%
Multi-wavelength
31%
T Tauri Stars
27%
Star Clusters
27%
Taurus
24%
Taiwanese Americans
24%
Quasars
23%
Proper Motions
22%
Nebulae
22%
Submillimeter
22%
B-field
22%
Young Stars
21%
Low-mass
21%
Outburst
20%
Luminosity
20%
Dust
20%
Multi-wavelength Observations
20%
Pre-main Sequence
20%
Fainting
20%
3C 454.3
19%
Young Stellar Objects
19%
Galaxies
19%
Emission Lines
19%
Comets
19%
Pulsation
18%
Lunar Occultation
17%
Mass Function
17%
Variable Stars
16%
Mrk 421
16%
Polarization Angle
16%
Magnetic Field Structure
15%
Massive Stars
14%
Pan-STARRS
14%
Polarimetric
14%
Physics
X Ray
100%
Blazars
90%
Light Curve
88%
Star Formation
75%
Photometry
64%
Magnetic Field
61%
Open Cluster
56%
Star Forming Regions
46%
Spectral Energy Distribution
44%
Near Infrared
43%
Synchrotron
37%
Star Cluster
36%
Quasar
34%
Molecular Clouds
33%
Trans-Neptunian Object
33%
Young Stellar Objects
26%
Proper Motion
24%
T Tauri Stars
23%
Observatory
23%
Optical Bursts
22%
Transients
22%
Circumstellar Disks
21%
Gamma Radiation
20%
Nebula
20%
Stellar Mass
19%
Lunar Occultation
19%
Sky Surveys
18%
Variable Star
16%
Stellar Classification
16%
Massive Star
16%
Extrasolar Planet
15%
Stellar Populations
15%
Energy Band
15%
Polarimetry
15%
Radial-Velocity Method
15%
Optical Property
14%
Young Star Clusters
13%
Classical T Tauri Stars
13%
Field of View
13%
Low-Mass Star
13%
Fermi Gamma-Ray Space Telescope
13%
Globular Cluster
12%
Star Distribution
12%
Active Galactic Nuclei
12%
X Ray Source
12%
Protostars
11%
Pre-Main Sequence Stars
11%
Kuiper Belt
11%
Light Emission
11%
Infrared Excess
10%
