G. E. Hassel

709 total citations
20 papers, 359 citations indexed

About

G. E. Hassel is a scholar working on Astronomy and Astrophysics, Spectroscopy and Atmospheric Science. According to data from OpenAlex, G. E. Hassel has authored 20 papers receiving a total of 359 indexed citations (citations by other indexed papers that have themselves been cited), including 16 papers in Astronomy and Astrophysics, 9 papers in Spectroscopy and 8 papers in Atmospheric Science. Recurrent topics in G. E. Hassel's work include Astrophysics and Star Formation Studies (16 papers), Molecular Spectroscopy and Structure (9 papers) and Atmospheric Ozone and Climate (8 papers). G. E. Hassel is often cited by papers focused on Astrophysics and Star Formation Studies (16 papers), Molecular Spectroscopy and Structure (9 papers) and Atmospheric Ozone and Climate (8 papers). G. E. Hassel collaborates with scholars based in United States, France and Sweden. G. E. Hassel's co-authors include Eric Herbst, J. H. Black, Maryvonne Gérin, Kinsuk Acharyya, K. M. Menten, Rose Finn, Edwin A. Bergin, J. R. Goicoechea, C. M. Persson and B. Mookerjea and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and Physical Review Physics Education Research.

In The Last Decade

G. E. Hassel

18 papers receiving 349 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
G. E. Hassel United States 12 241 198 137 131 35 20 359
W. M. Schlingman United States 9 325 1.3× 104 0.5× 10 0.1× 35 0.3× 51 1.5× 10 385
M. S. Kirsanova Russia 10 284 1.2× 84 0.4× 41 0.3× 60 0.5× 3 0.1× 36 297
John A. Milsom United States 8 246 1.0× 24 0.1× 51 0.4× 36 0.3× 7 0.2× 16 340
G. H. Bowen United States 10 613 2.5× 29 0.1× 24 0.2× 31 0.2× 15 0.4× 17 670
C. M. Persson Sweden 11 268 1.1× 177 0.9× 97 0.7× 125 1.0× 30 344
Liton Majumdar India 14 344 1.4× 288 1.5× 166 1.2× 144 1.1× 46 418
F. Peter Schloerb United States 4 233 1.0× 113 0.6× 78 0.6× 98 0.7× 7 264
Edouard Hugo Germany 8 209 0.9× 303 1.5× 280 2.0× 126 1.0× 12 463
M. Kamińska Sweden 9 223 0.9× 214 1.1× 207 1.5× 96 0.7× 12 343
M. Ikeda Japan 5 212 0.9× 240 1.2× 144 1.1× 126 1.0× 6 300

Countries citing papers authored by G. E. Hassel

Since Specialization
Citations

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

Fields of papers citing papers by G. E. Hassel

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. E. Hassel. 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 G. E. Hassel. The network helps show where G. E. Hassel may publish in the future.

Co-authorship network of co-authors of G. E. Hassel

This figure shows the co-authorship network connecting the top 25 collaborators of G. E. Hassel. A scholar is included among the top collaborators of G. E. Hassel 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 G. E. Hassel. G. E. Hassel 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.
Hassel, G. E., et al.. (2024). MSM Framework: AR Model of the Force on a Charge Moving in a Magnetic Field. The Physics Video Demonstration Database (Cornell University). 274–279.
2.
Hassel, G. E., et al.. (2023). Augmented Reality to Scaffold 2D Representations of 3D Models in Magnetism. The Physics Video Demonstration Database (Cornell University). 211–216.
3.
Christian, Matthew S., et al.. (2017). A New Take on Exploding Carts. The Physics Teacher. 55(8). 475–479. 1 indexed citations
4.
Finn, Rose, et al.. (2017). Assessing students’ conceptual knowledge of electricity and magnetism. Physical Review Physics Education Research. 13(2). 38 indexed citations
5.
Quan, Donghui, et al.. (2016). CHEMICAL SIMULATIONS OF PREBIOTIC MOLECULES: INTERSTELLAR ETHANIMINE ISOMERS. The Astrophysical Journal. 824(2). 129–129. 23 indexed citations
6.
Persson, Carina M., Romane Le Gal, E. S. Wirström, et al.. (2015). Ortho-to-para ratio of NH2. Astronomy and Astrophysics. 586. A128–A128. 11 indexed citations
7.
Crockett, N. R., Edwin A. Bergin, Justin L. Neill, et al.. (2015). HERSCHELOBSERVATIONS OF EXTRAORDINARY SOURCES: ANALYSIS OF THE HIFI 1.2 THz WIDE SPECTRAL SURVEY TOWARD ORION KL II. CHEMICAL IMPLICATIONS. The Astrophysical Journal. 806(2). 239–239. 23 indexed citations
8.
Mookerjea, B., C. Vastel, G. E. Hassel, et al.. (2014). Detection of a dense clump in a filament interacting with W51e2. Springer Link (Chiba Institute of Technology). 9 indexed citations
9.
Persson, C. M., G. E. Hassel, A. O. H. Olofsson, et al.. (2014). Upper limits to interstellar NH+and para-NH2−abundances. Astronomy and Astrophysics. 567. A130–A130. 18 indexed citations
10.
Persson, C. M., Maryvonne Gérin, B. Mookerjea, et al.. (2014). First detection of [N II] 205μm absorption in interstellar gas. Astronomy and Astrophysics. 568. A37–A37. 10 indexed citations
11.
Persson, C. M., G. E. Hassel, A. O. H. Olofsson, et al.. (2014). Upper limits to interstellar NH+ and para-NH2- abundances. Herschel-HIFI observations towards Sgr B2 (M) and G10.6-0.4 (W31C). Kölner Universitäts PublikationsServer (Universität zu Köln). 14 indexed citations
12.
Persson, C. M., Maryvonne Gérin, B. Mookerjea, et al.. (2014). First detection of [N II] 205 μm absorption in interstellar gas - Herschel-HIFI observations towards W 31C, W 49N, W 51, and G34.3+0.1. Chalmers Publication Library (Chalmers University of Technology). 568. 37. 5 indexed citations
13.
Mookerjea, B., G. E. Hassel, Maryvonne Gérin, et al.. (2012). Chemistry of C3and carbon chain molecules in DR21(OH). Astronomy and Astrophysics. 546. A75–A75. 27 indexed citations
14.
Persson, C. M., M. De Luca, B. Mookerjea, et al.. (2012). Nitrogen hydrides in interstellar gas. Astronomy and Astrophysics. 543. A145–A145. 55 indexed citations
15.
Persson, C. M., M. De Luca, B. Mookerjea, et al.. (2012). Nitrogen hydrides in interstellar gas II. Analysis of Herschel/HIFI observations towards W49N and G10.6-0.4 (W31C). UCL Discovery (University College London). 40 indexed citations
16.
Acharyya, Kinsuk, G. E. Hassel, & Eric Herbst. (2011). THE EFFECTS OF GRAIN SIZE AND GRAIN GROWTH ON THE CHEMICAL EVOLUTION OF COLD DENSE CLOUDS. The Astrophysical Journal. 732(2). 73–73. 34 indexed citations
17.
Hassel, G. E., Eric Herbst, & Edwin A. Bergin. (2010). Beyond the pseudo-time-dependent approach: chemical models of dense core precursors. Springer Link (Chiba Institute of Technology). 17 indexed citations
18.
Quan, Donghui, Eric Herbst, T. J. Millar, et al.. (2008). New Theoretical Results Concerning the Interstellar Abundance of Molecular Oxygen. The Astrophysical Journal. 681(2). 1318–1326. 28 indexed citations
19.
Hassel, G. E., W. G. Roberge, D. C. B. Whittet, & S. Shenoy. (2003). Shock processing of icy grain mantles in protoplanetary disks. 788. 1 indexed citations
20.
Shenoy, S., D. C. B. Whittet, J. E. Chiar, et al.. (2003). A Test Case for the Organic Refractory Model of Interstellar Dust. The Astrophysical Journal. 591(2). 962–967. 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.

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