S. R. Spangler

4.0k total citations · 1 hit paper
120 papers, 2.6k citations indexed

About

S. R. Spangler is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Computational Mechanics. According to data from OpenAlex, S. R. Spangler has authored 120 papers receiving a total of 2.6k indexed citations (citations by other indexed papers that have themselves been cited), including 113 papers in Astronomy and Astrophysics, 39 papers in Nuclear and High Energy Physics and 16 papers in Computational Mechanics. Recurrent topics in S. R. Spangler's work include Solar and Space Plasma Dynamics (62 papers), Ionosphere and magnetosphere dynamics (36 papers) and Astrophysics and Cosmic Phenomena (32 papers). S. R. Spangler is often cited by papers focused on Solar and Space Plasma Dynamics (62 papers), Ionosphere and magnetosphere dynamics (36 papers) and Astrophysics and Cosmic Phenomena (32 papers). S. R. Spangler collaborates with scholars based in United States, Italy and Puerto Rico. S. R. Spangler's co-authors include J. W. Armstrong, B. J. Rickett, Anthony H. Minter, J. P. Sheerin, J. M. Cordes, Salvatore Mancuso, S. T. Myers, C. R. Gwinn, A. Bhattacharjee and C. S. Ng and has published in prestigious journals such as Nature, SHILAP Revista de lepidopterología and Journal of Geophysical Research Atmospheres.

In The Last Decade

S. R. Spangler

108 papers receiving 2.4k 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.

Electron density power spectrum in the local interstellar medium

1995 539 citations S. R. Spangler et al. The Astrophysical Journal profile →

Peers

S. R. Spangler

AA

NHEP

MB

AMPO

CM

Ethan T. Vishniac United States

Petr Hellinger Czechia

A. Mangeney France

J. Heyvaerts France

Tohru Hada Japan

L. Vlahos Greece

L. Mestel United Kingdom

R. Beck Germany

Leaf Turner United States

I. W. Roxburgh United Kingdom

Ethan T. Vishniac United States

S. R. Spangler

3.0k ×1.2

AA

1.2k ×1.3

NHEP

460 ×1.4

MB

103 ×0.6

AMPO

204 ×1.5

CM

Citations per year, relative to S. R. Spangler S. R. Spangler (= 1×) peers Ethan T. Vishniac

Countries citing papers authored by S. R. Spangler

Since Specialization

Citations

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

Fields of papers citing papers by S. R. Spangler

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by S. R. Spangler. 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 S. R. Spangler. The network helps show where S. R. Spangler may publish in the future.

Co-authorship network of co-authors of S. R. Spangler

This figure shows the co-authorship network connecting the top 25 collaborators of S. R. Spangler. A scholar is included among the top collaborators of S. R. Spangler 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 S. R. Spangler. S. R. Spangler 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

1.

Spangler, S. R.. (2025). Broadening of the Main Sequence of a Star Cluster by Undetected Binaries. Research Notes of the AAS. 9(2). 34–34. 1 indexed citations

2.

Spangler, S. R.. (2022). On the Measurement of Vorticity in Astrophysical Fluids. Research Notes of the AAS. 6(10). 205–205. 1 indexed citations

3.

Ocker, Stella Koch, J. M. Cordes, Shami Chatterjee, et al.. (2021). Persistent plasma waves in interstellar space detected by Voyager 1. Nature Astronomy. 5(8). 761–765. 21 indexed citations

4.

Spangler, S. R.. (2020). Comparison of Radioastronomical Estimates of the Coronal and Solar Wind Magnetic Field with Measurements from Parker Solar Probe. Research Notes of the AAS. 4(8). 147–147. 2 indexed citations

5.

Chat, Gaétan Le, J. C. Kasper, Ofer Cohen, & S. R. Spangler. (2014). DIAGNOSTICS OF THE SOLAR CORONA FROM COMPARISON BETWEEN FARADAY ROTATION MEASUREMENTS AND MAGNETOHYDRODYNAMIC SIMULATIONS. The Astrophysical Journal. 789(2). 163–163. 4 indexed citations

6.

Spangler, S. R.. (2007). The Propagation Distance and Sources of Interstellar Turbulence. ASPC. 365. 307. 1 indexed citations

7.

Spangler, S. R.. (2003). The magnitude of heating of the Diffuse Ionized Gas of the interstellar medium by Landau damping of turbulence. Astronomy and Astrophysics. 407(2). 563–571. 3 indexed citations

8.

Spangler, S. R.. (2003). The small amplitude of density turbulence in the inner solar wind. SHILAP Revista de lepidopterología. 1 indexed citations

9.

Spangler, S. R., et al.. (2002). Very Long Baseline Interferometer measurements of turbulence in the inner solar wind. Astronomy and Astrophysics. 384(2). 654–665. 17 indexed citations

10.

Spangler, S. R.. (2002). The Amplitude of Magnetohydrodynamic Turbulence in the Inner Solar Wind. The Astrophysical Journal. 576(2). 997–1004. 35 indexed citations

11.

Bondi, M., et al.. (1994). One-year modulation in the flux density time series of low frequency variables.. A&A. 287. 390–402.

12.

Minter, Anthony H. & S. R. Spangler. (1992). Precision correction of radioastronomical polarization measurements for ionospheric faraday rotation. 180. 1 indexed citations

13.

Weisberg, J. M., Rachel A. Pildis, J. M. Cordes, S. R. Spangler, & Timothy Clifton. (1990). Interstellar Scattering in the Inner Galaxy. Bulletin of the American Astronomical Society. 22. 1244. 2 indexed citations

14.

Mantovani, F., R. Fanti, L. Gregorini, L. Padrielli, & S. R. Spangler. (1990). Interstellar medium parameters derived from the variability of radio sources at low frequencies.. 233(2). 535–539. 1 indexed citations

15.

Spangler, S. R., et al.. (1989). On evidence for quasi-parallel and quasi-perpendicular acceleration in supernova remnants. The Astrophysical Journal. 338. 963–963. 5 indexed citations

16.

Cordes, J. M., S. R. Spangler, J. M. Weisberg, & Timothy Clifton. (1988). Galactic distribution of electron density turbulence. AIP conference proceedings. 174. 180–184. 2 indexed citations

17.

Spangler, S. R.. (1984). Nonlinear evolution of astrophysical Alfven waves. NASA Technical Reports Server (NASA). 207. 197. 1 indexed citations

18.

Spangler, S. R., et al.. (1982). Green-Bank Workshop on Low Frequency Variability. 7. 4.

19.

Spangler, S. R., John M. Benson, J. M. Cordes, et al.. (1981). Dual-frequency VLBI observations of extragalactic sources with distinctive radio spectra. The Astronomical Journal. 86. 1155–1155. 1 indexed citations

20.

Cotton, W. D. & S. R. Spangler. (1975). Low Frequency Variability in Extragalactic Radio Sources. Bulletin of the American Astronomical Society. 7. 528. 5 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.

Explore authors with similar magnitude of impact