Y.‐M. Wang

2.2k total citations · 1 hit paper
19 papers, 1.5k 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 19 papers receiving a total of 1.5k indexed citations (citations by other indexed papers that have themselves been cited), including 19 papers in Astronomy and Astrophysics, 3 papers in Molecular Biology and 1 paper in Oceanography. Recurrent topics in Y.‐M. Wang's work include Solar and Space Plasma Dynamics (19 papers), Astro and Planetary Science (17 papers) and Stellar, planetary, and galactic studies (13 papers). Y.‐M. Wang is often cited by papers focused on Solar and Space Plasma Dynamics (19 papers), Astro and Planetary Science (17 papers) and Stellar, planetary, and galactic studies (13 papers). Y.‐M. Wang collaborates with scholars based in United States, United Kingdom and France. Y.‐M. Wang's co-authors include N. R. Sheeley, N. Rich, O. C. St. Cyr, R. A. Howard, D. G. Socker, A. Llébaria, D. J. Michels, G. E. Brueckner, G. M. Simnett and Harry P. Warren 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

19 papers receiving 1.5k citations

Hit Papers

align trajectories

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

Measurements of Flow Speeds in the Corona Between 2 and 30R_☉

1997 410 citations N. R. Sheeley, Y.‐M. Wang et al. The Astrophysical Journal profile →

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
Y.‐M. Wang United States	17	1.5k	364	111	59	34	19	1.5k
V. J. Pizzo United States	20	1.8k 1.2×	487 1.3×	91 0.8×	97 1.6×	71 2.1×	43	1.8k
Cooper Downs United States	23	1.3k 0.8×	285 0.8×	138 1.2×	54 0.9×	41 1.2×	70	1.3k
G. J. D. Petrie United States	19	1.2k 0.8×	396 1.1×	104 0.9×	45 0.8×	22 0.6×	66	1.2k
V. Archontis United Kingdom	25	1.8k 1.2×	573 1.6×	96 0.9×	39 0.7×	20 0.6×	54	1.8k
H. J. Hagenaar United States	14	1.1k 0.7×	355 1.0×	148 1.3×	22 0.4×	29 0.9×	22	1.1k
N. M. Viall United States	21	914 0.6×	325 0.9×	125 1.1×	39 0.7×	27 0.8×	50	967
J. Burkepile United States	23	1.8k 1.2×	433 1.2×	144 1.3×	53 0.9×	31 0.9×	60	1.9k
R. D’Amicis Italy	19	919 0.6×	469 1.3×	83 0.7×	28 0.5×	21 0.6×	60	943
Bidya Binay Karak India	19	962 0.6×	447 1.2×	82 0.7×	75 1.3×	24 0.7×	45	1.0k
E. Robbrecht Belgium	13	1.1k 0.7×	309 0.8×	144 1.3×	34 0.6×	28 0.8×	23	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

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19 of 19 papers shown

Owens, M. J., E. W. Cliver, K. G. McCracken, et al.. (2016). Near‐Earth heliospheric magnetic field intensity since 1750: 2. Cosmogenic radionuclide reconstructions. Journal of Geophysical Research Space Physics. 121(7). 6064–6074. 16 indexed citations

Burlaga, L. F., N. F. Ness, M. H. Acuña, Y.‐M. Wang, & N. R. Sheeley. (2009). Radial and solar cycle variations of the magnetic fields in the heliosheath: Voyager 1 observations from 2005 to 2008. Journal of Geophysical Research Atmospheres. 114(A6). 17 indexed citations

Burlaga, L. F., N. F. Ness, M. H. Acuña, et al.. (2008). Global structure and dynamics of large‐scale fluctuations in the solar wind: Voyager 2 observations during 2005 and 2006. Journal of Geophysical Research Atmospheres. 113(A2). 4 indexed citations

Wang, Y.‐M., N. R. Sheeley, & N. Rich. (2007). Coronal Pseudostreamers. The Astrophysical Journal. 658(2). 1340–1348. 149 indexed citations

Wang, Y.‐M., et al.. (2006). Role of the Sun’s Nonaxisymmetric Open Flux in Cosmic‐Ray Modulation. The Astrophysical Journal. 644(1). 638–645. 32 indexed citations

Wang, Y.‐M. & N. R. Sheeley. (2006). Sources of the Solar Wind atUlyssesduring 1990–2006. The Astrophysical Journal. 653(1). 708–718. 28 indexed citations

Sheeley, N. R., Harry P. Warren, & Y.‐M. Wang. (2004). The Origin of Postflare Loops. The Astrophysical Journal. 616(2). 1224–1231. 76 indexed citations

Wang, Y.‐M. & N. R. Sheeley. (2004). Footpoint Switching and the Evolution of Coronal Holes. The Astrophysical Journal. 612(2). 1196–1205. 68 indexed citations

Whang, Y. C., et al.. (2003). Solar Wind Speed and Temperature Outside 10 AU and the Termination Shock. The Astrophysical Journal. 589(1). 635–643. 21 indexed citations

10.

Wang, Y.‐M. & N. R. Sheeley. (2003). On the Fluctuating Component of the Sun’s Large‐Scale Magnetic Field. The Astrophysical Journal. 590(2). 1111–1120. 81 indexed citations

11.

Wang, Y.‐M., et al.. (2003). The Solar Wind and Its Magnetic Sources at Sunspot Maximum. The Astrophysical Journal. 587(2). 818–822. 45 indexed citations

12.

Sheeley, N. R. & Y.‐M. Wang. (2002). Characteristics of Coronal Inflows. The Astrophysical Journal. 579(2). 874–887. 65 indexed citations

13.

Wang, Y.‐M., N. R. Sheeley, & J. Lean. (2002). Meridional Flow and the Solar Cycle Variation of the Sun’s Open Magnetic Flux. The Astrophysical Journal. 580(2). 1188–1196. 66 indexed citations

14.

Wang, Y.‐M., et al.. (2002). Coronal White‐Light Jets near Sunspot Maximum. The Astrophysical Journal. 575(1). 542–552. 57 indexed citations

15.

Wang, Y.‐M.. (2001). On the Relationship between Heiiλ304 Prominences and the Photospheric Magnetic Field. The Astrophysical Journal. 560(1). 456–465. 48 indexed citations

16.

Wang, Y.‐M., N. R. Sheeley, R. A. Howard, O. C. St. Cyr, & G. M. Simnett. (1999). Coronagraph observations of inflows during high solar activity. Geophysical Research Letters. 26(9). 1203–1206. 59 indexed citations

17.

Neugebauer, M., R. J. Forsyth, A. B. Galvin, et al.. (1998). Spatial structure of the solar wind and comparisons with solar data and models. Journal of Geophysical Research Atmospheres. 103(A7). 14587–14599. 170 indexed citations

18.

Wang, Y.‐M., D. G. Socker, R. A. Howard, et al.. (1998). Observations of Correlated White‐Light and Extreme‐Ultraviolet Jets from Polar Coronal Holes. The Astrophysical Journal. 508(2). 899–907. 125 indexed citations

19.

Sheeley, N. R., Y.‐M. Wang, Scott H. Hawley, et al.. (1997). Measurements of Flow Speeds in the Corona Between 2 and 30R_☉. The Astrophysical Journal. 484(1). 472–478. 410 indexed citations breakdown →

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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