Chung‐Ming Ko

1.0k total citations
71 papers, 675 citations indexed

About

Chung‐Ming Ko is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Atomic and Molecular Physics, and Optics. According to data from OpenAlex, Chung‐Ming Ko has authored 71 papers receiving a total of 675 indexed citations (citations by other indexed papers that have themselves been cited), including 64 papers in Astronomy and Astrophysics, 40 papers in Nuclear and High Energy Physics and 5 papers in Atomic and Molecular Physics, and Optics. Recurrent topics in Chung‐Ming Ko's work include Solar and Space Plasma Dynamics (37 papers), Astrophysics and Cosmic Phenomena (36 papers) and Astrophysics and Star Formation Studies (20 papers). Chung‐Ming Ko is often cited by papers focused on Solar and Space Plasma Dynamics (37 papers), Astrophysics and Cosmic Phenomena (36 papers) and Astrophysics and Star Formation Studies (20 papers). Chung‐Ming Ko collaborates with scholars based in Taiwan, Russia and Hong Kong. Chung‐Ming Ko's co-authors include G. M. Webb, V. A. Dogiel, D. O. Chernyshov, K. S. Cheng, W.-H. Ip, Zi-Wei Lin, Wei Liu, G. P. Zank, J. R. Jokipii and Kenji Nakamura and has published in prestigious journals such as SHILAP Revista de lepidopterología, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

Chung‐Ming Ko

57 papers receiving 631 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
Chung‐Ming Ko Taiwan 16 554 414 33 29 8 71 675
C. L. Carilli United States 13 652 1.2× 341 0.8× 76 2.3× 23 0.8× 5 0.6× 22 671
A. Berdyugin Finland 17 675 1.2× 253 0.6× 65 2.0× 17 0.6× 12 1.5× 62 721
Subhashis Roy India 12 516 0.9× 285 0.7× 21 0.6× 23 0.8× 6 0.8× 28 532
S. D. Vergani France 16 804 1.5× 209 0.5× 88 2.7× 21 0.7× 6 0.8× 68 831
E. Fürst Germany 15 644 1.2× 407 1.0× 20 0.6× 9 0.3× 18 2.3× 35 666
H. Álvarez Chile 10 390 0.7× 161 0.4× 13 0.4× 15 0.5× 15 1.9× 31 421
Bhargav Vaidya India 16 636 1.1× 421 1.0× 22 0.7× 10 0.3× 27 3.4× 58 693
Anthony H. Minter United States 10 440 0.8× 195 0.5× 8 0.2× 21 0.7× 15 1.9× 23 461
Rishi Khatri India 14 412 0.7× 289 0.7× 18 0.5× 17 0.6× 2 0.3× 31 455
Sean M. Couch United States 22 1.1k 2.0× 709 1.7× 44 1.3× 23 0.8× 6 0.8× 40 1.3k

Countries citing papers authored by Chung‐Ming Ko

Since Specialization
Citations

This map shows the geographic impact of Chung‐Ming Ko's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by Chung‐Ming Ko with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Chung‐Ming Ko more than expected).

Fields of papers citing papers by Chung‐Ming Ko

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Chung‐Ming Ko. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by Chung‐Ming Ko. The network helps show where Chung‐Ming Ko may publish in the future.

Co-authorship network of co-authors of Chung‐Ming Ko

This figure shows the co-authorship network connecting the top 25 collaborators of Chung‐Ming Ko. A scholar is included among the top collaborators of Chung‐Ming Ko based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with Chung‐Ming Ko. Chung‐Ming Ko is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Ko, Chung‐Ming, et al.. (2024). A distinct radial acceleration relation across the brightest cluster galaxies and galaxy clusters. Astronomy and Astrophysics. 684. A180–A180. 5 indexed citations
2.
Li, Pengfei, Marcel S. Pawlowski, Federico Lelli, et al.. (2023). Measuring galaxy cluster mass profiles into the low-acceleration regime with galaxy kinematics. Astronomy and Astrophysics. 677. A24–A24. 15 indexed citations
3.
Ko, Chung‐Ming, et al.. (2023). Classifying MaNGA velocity dispersion profiles by machine learning. Research at the University of Copenhagen (University of Copenhagen). 2(1). 649–656. 1 indexed citations
4.
Cheng, Han, et al.. (2021). Mass–Velocity Dispersion Relation in MaNGA Brightest Cluster Galaxies. The Astrophysical Journal Letters. 917(2). L24–L24. 7 indexed citations
5.
Ko, Chung‐Ming, et al.. (2021). Cosmic ray propagation with cosmic ray viscosity in hydrodynamic description. 43. 1381. 2 indexed citations
6.
Ko, Chung‐Ming, et al.. (2021). Outflows in the presence of cosmic rays and waves with cooling. Astronomy and Astrophysics. 654. A63–A63. 5 indexed citations
7.
Ko, Chung‐Ming, et al.. (2018). Structure of interstellar clouds including the effects of cosmic rays and waves. cosp. 42. 2 indexed citations
8.
Hwang, Chorng‐Yuan, et al.. (2016). ELLIPTICITIES OF ELLIPTICAL GALAXIES IN DIFFERENT ENVIRONMENTS. The Astrophysical Journal. 830(2). 123–123. 4 indexed citations
9.
Dogiel, V. A., D. O. Chernyshov, A. M. Kiselev, et al.. (2015). SPECTRUM OF RELATIVISTIC AND SUBRELATIVISTIC COSMIC RAYS IN THE 100 pc CENTRAL REGION. The Astrophysical Journal. 809(1). 48–48. 14 indexed citations
10.
Ko, Chung‐Ming, V. A. Dogiel, D. O. Chernyshov, & K. S. Cheng. (2014). Multi-wavelength emission from the Fermi Bubbles. 40.
11.
Cheng, K. S., et al.. (2012). THE FERMI BUBBLE AS A SOURCE OF COSMIC RAYS IN THE ENERGY RANGE >1015eV. The Astrophysical Journal. 746(2). 116–116. 20 indexed citations
12.
Chernyshov, D. O., K. S. Cheng, V. A. Dogiel, Chung‐Ming Ko, & W.-H. Ip. (2010). Restrictions on the injection energy of positrons annihilating near the Galactic Centre. Monthly Notices of the Royal Astronomical Society. 403(2). 817–825. 5 indexed citations
13.
Dogiel, V. A., V. Tatischeff, K. S. Cheng, et al.. (2009). Nuclear interaction gamma-ray lines from the Galactic center region. Springer Link (Chiba Institute of Technology). 14 indexed citations
14.
Dogiel, V. A., K. S. Cheng, D. O. Chernyshov, et al.. (2008). De-excitation C and O lines and the 511keV annihilation line from Sgr A∗. New Astronomy Reviews. 52(7-10). 460–462. 3 indexed citations
15.
Ko, Chung‐Ming, et al.. (2007). Stability of a system with cosmic rays and waves. Astronomy and Astrophysics. 469(3). 829–837. 3 indexed citations
16.
Dogiel, V. A., S. Colafrancesco, Chung‐Ming Ko, et al.. (2006). In-situ acceleration of subrelativistic electrons in the Coma halo and the halo's influence on the Sunyaev-Zeldovich effect. Springer Link (Chiba Institute of Technology). 18 indexed citations
17.
Ko, Chung‐Ming. (2001). Hydrodynamic approach to cosmic ray acceleration. Journal of The Korean Astronomical Society. 34(4). 289–291. 2 indexed citations
18.
Ko, Chung‐Ming & E. N. Parker. (1989). Intermittent behavior of galactic dynamo activities. The Astrophysical Journal. 341. 828–828. 16 indexed citations
19.
Ko, Chung‐Ming, J. R. Jokipii, & G. M. Webb. (1987). Cosmic-Ray Modified Stellar Winds. International Cosmic Ray Conference. 2. 191. 2 indexed citations
20.
Ko, Chung‐Ming & J. R. Jokipii. (1985). A numerical study of diffusive shock acceleration of cosmic rays in supernova shocks. NASA STI Repository (National Aeronautics and Space Administration). 3. 156.

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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