Y.‐M. Wang

3.2k total citations · 1 hit paper
28 papers, 2.3k citations indexed

About

Y.‐M. Wang is a scholar working on Astronomy and Astrophysics, Molecular Biology and Oceanography. According to data from OpenAlex, Y.‐M. Wang has authored 28 papers receiving a total of 2.3k indexed citations (citations by other indexed papers that have themselves been cited), including 28 papers in Astronomy and Astrophysics, 7 papers in Molecular Biology and 1 paper in Oceanography. Recurrent topics in Y.‐M. Wang's work include Solar and Space Plasma Dynamics (28 papers), Astro and Planetary Science (17 papers) and Stellar, planetary, and galactic studies (15 papers). Y.‐M. Wang is often cited by papers focused on Solar and Space Plasma Dynamics (28 papers), Astro and Planetary Science (17 papers) and Stellar, planetary, and galactic studies (15 papers). Y.‐M. Wang collaborates with scholars based in United States, France and Germany. Y.‐M. Wang's co-authors include N. R. Sheeley, J. Lean, R. A. Howard, Jada Walters, M. Pick, G. M. Mason, D. G. Socker, N. Rich, L. F. Burlaga and K. Muglach and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, The Astrophysical Journal and Geophysical Research Letters.

In The Last Decade

Y.‐M. Wang

28 papers receiving 2.2k citations

Hit Papers

Modeling the Sun’s Magnetic Field and Irradiance since 1713 2005 2026 2012 2019 2005 100 200 300 400

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Y.‐M. Wang United States 24 2.0k 507 357 292 192 28 2.3k
Yu. A. Nagovitsyn Russia 18 945 0.5× 341 0.7× 287 0.8× 207 0.7× 180 0.9× 104 1.2k
Luke Barnard United Kingdom 24 1.3k 0.7× 656 1.3× 234 0.7× 141 0.5× 159 0.8× 84 1.5k
A. I. Shapiro Germany 24 1.3k 0.7× 103 0.2× 790 2.2× 501 1.7× 310 1.6× 98 1.9k
K. Tziotziou Greece 22 1.1k 0.5× 183 0.4× 93 0.3× 80 0.3× 234 1.2× 51 1.2k
S. M. Silverman United States 20 1.1k 0.5× 397 0.8× 373 1.0× 181 0.6× 51 0.3× 77 1.3k
A. P. Rouillard France 33 2.8k 1.4× 911 1.8× 102 0.3× 45 0.2× 264 1.4× 97 2.8k
Margit Haberreiter Switzerland 16 799 0.4× 66 0.1× 488 1.4× 285 1.0× 322 1.7× 48 1.1k
M. Wild United Kingdom 15 1.0k 0.5× 555 1.1× 164 0.5× 119 0.4× 93 0.5× 31 1.1k
Nigel Marsh Denmark 8 446 0.2× 98 0.2× 493 1.4× 421 1.4× 89 0.5× 13 796
Christopher J. Scott United Kingdom 22 983 0.5× 423 0.8× 171 0.5× 109 0.4× 67 0.3× 78 1.1k

Countries citing papers authored by Y.‐M. Wang

Since Specialization
Citations

This map shows the geographic impact of Y.‐M. Wang'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 Y.‐M. Wang with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Y.‐M. Wang more than expected).

Fields of papers citing papers by Y.‐M. Wang

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Y.‐M. Wang. 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 Y.‐M. Wang. The network helps show where Y.‐M. Wang may publish in the future.

Co-authorship network of co-authors of Y.‐M. Wang

This figure shows the co-authorship network connecting the top 25 collaborators of Y.‐M. Wang. A scholar is included among the top collaborators of Y.‐M. Wang 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 Y.‐M. Wang. Y.‐M. Wang 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.
Burlaga, L. F., N. F. Ness, Y.‐M. Wang, N. R. Sheeley, & J. D. Richardson. (2010). Observations of the magnetic field and plasma in the heliosheath by Voyager 2 from 2007.7 to 2009.4. Journal of Geophysical Research Atmospheres. 115(A8). 13 indexed citations
2.
Wang, Y.‐M.. (2008). Relating the Solar Wind Helium Abundance to the Coronal Magnetic Field. The Astrophysical Journal. 683(1). 499–509. 23 indexed citations
3.
Sheeley, N. R. & Y.‐M. Wang. (2007). In/Out Pairs and the Detachment of Coronal Streamers. The Astrophysical Journal. 655(2). 1142–1156. 50 indexed citations
4.
Wang, Y.‐M. & K. Muglach. (2007). On the Formation of Filament Channels. The Astrophysical Journal. 666(2). 1284–1295. 57 indexed citations
5.
Wang, Y.‐M., M. Pick, & G. M. Mason. (2006). Coronal Holes, Jets, and the Origin of3He‐rich Particle Events. The Astrophysical Journal. 639(1). 495–509. 118 indexed citations
6.
Wang, Y.‐M. & N. R. Sheeley. (2006). Observations of Flux Rope Formation in the Outer Corona. The Astrophysical Journal. 650(2). 1172–1183. 27 indexed citations
7.
Wang, Y.‐M., J. Lean, & N. R. Sheeley. (2005). Modeling the Sun’s Magnetic Field and Irradiance since 1713. The Astrophysical Journal. 625(1). 522–538. 439 indexed citations breakdown →
8.
Whang, Y. C., L. F. Burlaga, Y.‐M. Wang, & N. R. Sheeley. (2004). The termination shock near 35° latitude. Geophysical Research Letters. 31(3). 23 indexed citations
9.
Wang, Y.‐M., et al.. (2003). On the Topological Evolution of the Coronal Magnetic Field During the Solar Cycle. The Astrophysical Journal. 599(2). 1404–1417. 50 indexed citations
10.
Lean, J., Y.‐M. Wang, & N. R. Sheeley. (2002). The effect of increasing solar activity on the Sun's total and open magnetic flux during multiple cycles: Implications for solar forcing of climate. Geophysical Research Letters. 29(24). 103 indexed citations
11.
Wang, Y.‐M. & N. R. Sheeley. (2002). Sunspot activity and the long‐term variation of the Sun's open magnetic flux. Journal of Geophysical Research Atmospheres. 107(A10). 78 indexed citations
12.
Wang, Y.‐M. & N. R. Sheeley. (2002). Observations of Core Fallback during Coronal Mass Ejections. The Astrophysical Journal. 567(2). 1211–1224. 20 indexed citations
13.
Burlaga, L. F., N. F. Ness, Y.‐M. Wang, & N. R. Sheeley. (2002). Heliospheric magnetic field strength and polarity from 1 to 81 AU during the ascending phase of solar cycle 23. Journal of Geophysical Research Atmospheres. 107(A11). 50 indexed citations
14.
Sheeley, N. R., et al.. (2000). Detection of coronal mass ejection associated shock waves in the outer corona. Journal of Geophysical Research Atmospheres. 105(A3). 5081–5092. 109 indexed citations
15.
Wang, Y.‐M., N. R. Sheeley, D. G. Socker, R. A. Howard, & N. Rich. (2000). The dynamical nature of coronal streamers. Journal of Geophysical Research Atmospheres. 105(A11). 25133–25142. 175 indexed citations
16.
Sheeley, N. R., Jada Walters, Y.‐M. Wang, & R. A. Howard. (1999). Continuous tracking of coronal outflows: Two kinds of coronal mass ejections. Journal of Geophysical Research Atmospheres. 104(A11). 24739–24767. 413 indexed citations
17.
Burlaga, L. F., N. F. Ness, Y.‐M. Wang, & N. R. Sheeley. (1998). Heliospheric magnetic field strength out to 66 AU: Voyager 1, 1978–1996. Journal of Geophysical Research Atmospheres. 103(A10). 23727–23732. 18 indexed citations
18.
Wang, Y.‐M. & N. R. Sheeley. (1997). The high‐latitude solar wind near sunspot Maximum. Geophysical Research Letters. 24(24). 3141–3144. 27 indexed citations
19.
Wang, Y.‐M., N. R. Sheeley, Scott H. Hawley, et al.. (1997). The Green Line Corona and Its Relation to the Photospheric Magnetic Field. The Astrophysical Journal. 485(1). 419–429. 49 indexed citations
20.
Wang, Y.‐M. & N. R. Sheeley. (1988). The solar origin of long‐term variations of the interplanetary magnetic field strength. Journal of Geophysical Research Atmospheres. 93(A10). 11227–11236. 59 indexed citations

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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