C. C. Cheng

1.0k total citations
40 papers, 695 citations indexed

About

C. C. Cheng is a scholar working on Astronomy and Astrophysics, Oceanography and Molecular Biology. According to data from OpenAlex, C. C. Cheng has authored 40 papers receiving a total of 695 indexed citations (citations by other indexed papers that have themselves been cited), including 34 papers in Astronomy and Astrophysics, 7 papers in Oceanography and 4 papers in Molecular Biology. Recurrent topics in C. C. Cheng's work include Solar and Space Plasma Dynamics (33 papers), Ionosphere and magnetosphere dynamics (20 papers) and Stellar, planetary, and galactic studies (8 papers). C. C. Cheng is often cited by papers focused on Solar and Space Plasma Dynamics (33 papers), Ionosphere and magnetosphere dynamics (20 papers) and Stellar, planetary, and galactic studies (8 papers). C. C. Cheng collaborates with scholars based in United States, Taiwan and France. C. C. Cheng's co-authors include U. Feldman, K. G. Widing, G. A. Doschek, G. A. Doschek, V. L. Jacobs, S. K. Antiochos, J. W. Cook, E. Tandberg‐Hanssen, J. T. Mariska and J. P. Boris and has published in prestigious journals such as The Astrophysical Journal, Geophysical Journal International and Electronics Letters.

In The Last Decade

C. C. Cheng

40 papers receiving 637 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
C. C. Cheng United States	17	599	99	74	74	52	40	695
A. Magun Switzerland	19	879 1.5×	160 1.6×	124 1.7×	57 0.8×	71 1.4×	75	966
И. В. Чашей Russia	15	902 1.5×	200 2.0×	108 1.5×	88 1.2×	57 1.1×	146	949
R. Reinhard Netherlands	15	801 1.3×	60 0.6×	224 3.0×	24 0.3×	57 1.1×	46	880
K. J. Frost United States	17	826 1.4×	134 1.4×	236 3.2×	46 0.6×	112 2.2×	44	890
A. Boischot France	15	1.1k 1.9×	295 3.0×	92 1.2×	46 0.6×	79 1.5×	46	1.1k
C. L. Hyder United States	14	468 0.8×	84 0.8×	29 0.4×	51 0.7×	15 0.3×	26	507
H. Koshiishi Japan	13	605 1.0×	183 1.8×	54 0.7×	54 0.7×	95 1.8×	35	716
A. R. Barakat United States	21	930 1.6×	188 1.9×	80 1.1×	44 0.6×	135 2.6×	51	1.0k
J. Solomon France	17	770 1.3×	153 1.5×	86 1.2×	22 0.3×	295 5.7×	35	813
D. E. Page Netherlands	10	421 0.7×	136 1.4×	34 0.5×	15 0.2×	39 0.8×	42	505

Countries citing papers authored by C. C. Cheng

Since Specialization

Citations

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

Fields of papers citing papers by C. C. Cheng

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by C. C. Cheng. 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 C. C. Cheng. The network helps show where C. C. Cheng may publish in the future.

Co-authorship network of co-authors of C. C. Cheng

This figure shows the co-authorship network connecting the top 25 collaborators of C. C. Cheng. A scholar is included among the top collaborators of C. C. Cheng 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 C. C. Cheng. C. C. Cheng is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Mouyen, Maxime, Martine Simões, Frédéric Mouthereau, et al.. (2014). Investigating possible gravity change rates expected from long-term deep crustal processes in Taiwan. Geophysical Journal International. 198(1). 187–197. 6 indexed citations

Hwang, Cheinway, et al.. (2009). Land subsidence using absolute and relative gravimetry: a case study in central Taiwan. Survey Review. 42(315). 27–39. 21 indexed citations

Luo, Guang-Li, C. C. Cheng, Chen‐Yu Huang, et al.. (2005). Suppressing phosphorus diffusion in germanium by carbon incorporation. Electronics Letters. 41(24). 1354–1355. 10 indexed citations

Wu, S. T., Minhang Song, C. C. Cheng, & M. Dryer. (1994). Coronal heating due to the emergence of magnetic flux. Space Science Reviews. 70(1-2). 167–170. 3 indexed citations

Cheng, C. C., et al.. (1993). Thermal and Nonthermal Energicatiosn in Solar Flares: Soft X-ray Spectroscopic and Hard X-ray Observations. 213–216. 1 indexed citations

Cerruti-Sola, M., C. C. Cheng, & R. Pallavicini. (1992). Mg II absolute line profiles for late-type stars and for spatially-resolved solar regions. 256(1). 185–194. 1 indexed citations

Cook, J. W., C. C. Cheng, V. L. Jacobs, & S. K. Antiochos. (1989). Effect of coronal elemental abundances on the radiative loss function. The Astrophysical Journal. 338. 1176–1176. 95 indexed citations

Cheng, C. C., L. E. Orwig, & E. Tandberg‐Hanssen. (1987). Temporal correlation between impulsive hard X-ray and UV bursts in flares observed with high time resolution. Solar Physics. 113(1-2). 301–302. 2 indexed citations

Pallavicini, R., et al.. (1986). The preheating of solar flares and reconnection. Advances in Space Research. 6(6). 69–71. 1 indexed citations

10.

Feldman, U., C. C. Cheng, & G. A. Doschek. (1982). Observational constraints for a theoretical model describing the soft X-ray flare. The Astrophysical Journal. 255. 320–320. 16 indexed citations

11.

Doschek, G. A., J. P. Boris, C. C. Cheng, J. T. Mariska, & E. S. Oran. (1982). A Numerical Simulation of Cooling Coronal Flare Plasma. The Astrophysical Journal. 258. 373–373. 16 indexed citations

12.

Cheng, C. C., R. G. Athay, J. M. Beckers, et al.. (1981). Preliminary observations and results obtained with the ultraviolet spectrometer and polarimeter. The Astrophysical Journal. 244. L127–L127. 17 indexed citations

13.

Tandberg‐Hanssen, E., C. C. Cheng, B. E. Woodgate, et al.. (1981). Solar maximum mission experiment: Ultraviolet spectroscopy and polarimetry on the solar maximum mission. Advances in Space Research. 1(13). 275–283. 5 indexed citations

14.

Canfield, R. C., C. C. Cheng, K. P. Dere, et al.. (1980). Radiative energy output of the 5 September 1973 flare. 451–469. 10 indexed citations

15.

Cheng, C. C.. (1980). Physical properties of individual coronal loops in a solar active region observed in the XUV. The Astrophysical Journal. 238. 743–743. 18 indexed citations

16.

Webb, D. F., C. C. Cheng, G. A. Dulk, et al.. (1980). Mechanical energy output of the 5 September 1973 flare. 471–499. 8 indexed citations

17.

Cheng, C. C., U. Feldman, & G. A. Doschek. (1979). The Fe XXI lambda1354 line in solar flares observed from SKYLAB and its implications on ionization equilibrium calculations. The Astrophysical Journal. 233. 736–736. 16 indexed citations

18.

Cheng, C. C., G. A. Doschek, & U. Feldman. (1979). The dynamical properties of the solar corona from intensities and line widths of EUV forbidden lines of SI VIII, Fe XI, and Fe XII. The Astrophysical Journal. 227. 1037–1037. 71 indexed citations

19.

Schmahl, E. J., et al.. (1978). The pre-onset morphology of the 5 September 1973 flare. Solar Physics. 60(2). 323–339. 10 indexed citations

20.

Widing, K. G. & C. C. Cheng. (1974). On the Fe XXIV emission in the solar flare of 1973 June 15. The Astrophysical Journal. 194. L111–L111. 36 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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