L. M. Haffner

2.5k total citations
55 papers, 1.4k citations indexed

About

L. M. Haffner is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Atmospheric Science. According to data from OpenAlex, L. M. Haffner has authored 55 papers receiving a total of 1.4k indexed citations (citations by other indexed papers that have themselves been cited), including 52 papers in Astronomy and Astrophysics, 13 papers in Nuclear and High Energy Physics and 12 papers in Atmospheric Science. Recurrent topics in L. M. Haffner's work include Astrophysics and Star Formation Studies (38 papers), Stellar, planetary, and galactic studies (29 papers) and Galaxies: Formation, Evolution, Phenomena (17 papers). L. M. Haffner is often cited by papers focused on Astrophysics and Star Formation Studies (38 papers), Stellar, planetary, and galactic studies (29 papers) and Galaxies: Formation, Evolution, Phenomena (17 papers). L. M. Haffner collaborates with scholars based in United States, United Kingdom and Australia. L. M. Haffner's co-authors include R. J. Reynolds, S. L. Tufte, G. J. Madsen, R. J. Reynolds, J. W. Percival, Kenneth Wood, Kurt P. Jaehnig, Alex S. Hill, R.‐J. Dettmar and Jonathan D. Slavin and has published in prestigious journals such as Journal of Geophysical Research Atmospheres, Reviews of Modern Physics and The Astrophysical Journal.

In The Last Decade

L. M. Haffner

53 papers receiving 1.3k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
L. M. Haffner United States 17 1.3k 314 103 75 75 55 1.4k
Troels Haugbølle Denmark 27 1.5k 1.1× 624 2.0× 101 1.0× 54 0.7× 151 2.0× 51 1.6k
A. B. Peck United States 23 1.6k 1.2× 429 1.4× 67 0.7× 140 1.9× 183 2.4× 54 1.6k
Jeremy Darling United States 23 1.1k 0.8× 350 1.1× 91 0.9× 123 1.6× 121 1.6× 74 1.2k
Jonathan D. Slavin United States 23 1.8k 1.3× 454 1.4× 105 1.0× 80 1.1× 34 0.5× 59 1.8k
G. J. Madsen Australia 16 1.2k 0.9× 418 1.3× 40 0.4× 86 1.1× 30 0.4× 34 1.3k
I. A. Grenier France 20 1.6k 1.2× 890 2.8× 161 1.6× 48 0.6× 145 1.9× 82 1.8k
J. May Chile 20 1.6k 1.2× 506 1.6× 147 1.4× 91 1.2× 261 3.5× 62 1.7k
Bon‐Chul Koo South Korea 25 1.6k 1.2× 772 2.5× 90 0.9× 47 0.6× 159 2.1× 93 1.7k
J. Kelly Truelove United States 4 1.1k 0.8× 330 1.1× 49 0.5× 63 0.8× 57 0.8× 5 1.2k
Michel Fich Canada 19 1.7k 1.3× 225 0.7× 166 1.6× 175 2.3× 302 4.0× 46 1.7k

Countries citing papers authored by L. M. Haffner

Since Specialization
Citations

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

Fields of papers citing papers by L. M. Haffner

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by L. M. Haffner. 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 L. M. Haffner. The network helps show where L. M. Haffner may publish in the future.

Co-authorship network of co-authors of L. M. Haffner

This figure shows the co-authorship network connecting the top 25 collaborators of L. M. Haffner. A scholar is included among the top collaborators of L. M. Haffner 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 L. M. Haffner. L. M. Haffner 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.
Wood, Kenneth, et al.. (2025). The Hα sky in three dimensions. Monthly Notices of the Royal Astronomical Society Letters. 540(1). L21–L27. 2 indexed citations
2.
Anderson, L. D., et al.. (2023). The GBT Diffuse Ionized Gas Survey (GDIGS): Discrete Sources. The Astrophysical Journal. 959(2). 110–110. 1 indexed citations
3.
Anderson, L. D., et al.. (2023). Methods for Averaging Spectral Line Data. Publications of the Astronomical Society of the Pacific. 135(1053). 114504–114504. 1 indexed citations
4.
Haffner, L. M., et al.. (2023). The Diffuse Ionized Gas Halo of the Large Magellanic Cloud. The Astrophysical Journal. 948(2). 118–118. 3 indexed citations
5.
Krishnarao, Dhanesh, Christy Tremonti, Amelia Fraser-McKelvie, et al.. (2020). The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs. The Astrophysical Journal. 898(2). 116–116. 13 indexed citations
6.
Anderson, L. D., et al.. (2020). The GBT Diffuse Ionized Gas Survey: Tracing the Diffuse Ionized Gas around the Giant Hii Region W43. The Astrophysical Journal. 889(2). 96–96. 6 indexed citations
7.
Nossal, S. M., et al.. (2019). Geocoronal Hydrogen Emission Variation Over Two Solar Cycles. Journal of Geophysical Research Space Physics. 124(12). 10674–10689. 4 indexed citations
8.
Jones, Amy, Guinevere Kauffmann, Richard D’Souza, et al.. (2016). SDSS IV MaNGA: Deep observations of extra-planar, diffuse ionized gas around late-type galaxies from stacked IFU spectra. Astronomy and Astrophysics. 599. A141–A141. 24 indexed citations
9.
Wood, Kenneth, J. E. Barnes, Barbara Ercolano, et al.. (2013). THREE-DIMENSIONAL GEOMETRIES AND THE ANALYSIS OF H II REGIONS. The Astrophysical Journal. 770(2). 152–152. 4 indexed citations
10.
Barger, Kathleen A., et al.. (2012). PRESENT-DAY GALACTIC EVOLUTION: LOW-METALLICITY, WARM, IONIZED GAS INFLOW ASSOCIATED WITH HIGH-VELOCITY CLOUD COMPLEX A. The Astrophysical Journal. 761(2). 145–145. 11 indexed citations
11.
Hill, Alex S., M. Joung, Robert A. Benjamin, et al.. (2011). MHD Simulations of a Supernova-driven ISM and the Warm Ionized Medium. 217. 1 indexed citations
12.
Haffner, L. M., R. J. Reynolds, G. J. Madsen, et al.. (2010). Early Results from the Wisconsin H-Alpha Mapper Southern Sky Survey. Scholarly Commons (Embry–Riddle Aeronautical University). 215. 388–392. 4 indexed citations
13.
Hill, Alex S., L. M. Haffner, & Ronald J. Reynolds. (2009). IONIZED GAS IN THE SMITH CLOUD. The Astrophysical Journal. 703(2). 1832–1838. 28 indexed citations
14.
Haffner, L. M., R.‐J. Dettmar, J. E. Beckman, et al.. (2009). The warm ionized medium in spiral galaxies. Reviews of Modern Physics. 81(3). 969–997. 202 indexed citations
15.
Madsen, G. J., R. J. Reynolds, & L. M. Haffner. (2006). A Multiwavelength Optical Emission Line Survey of Warm Ionized Gas in the Galaxy. The Astrophysical Journal. 652(1). 401–425. 96 indexed citations
16.
Reynolds, R. J., N. C. Sterling, & L. M. Haffner. (2001). Detection of a Large Arc of Ionized Hydrogen Far above the Cassiopeia OB6 Association: A Superbubble Blowout into the Galactic Halo?. The Astrophysical Journal. 558(2). L101–L104. 31 indexed citations
17.
Reynolds, R. J., et al.. (2000). TEMPERATURE VARIATIONS AND NON-PHOTOIONIZATION HEATING IN THE WARM IONIZED MEDIUM OF GALAXIES. 9. 249–255. 2 indexed citations
18.
Haffner, L. M., R. J. Reynolds, & S. L. Tufte. (2000). The wisconsin Ha mapper:a new look at the warm ionized medium. 9. 238–245. 2 indexed citations
19.
Heiles, Carl, L. M. Haffner, & R. J. Reynolds. (1999). The Eridanus Superbubble in its Multiwavelength Glory. 168. 211. 4 indexed citations
20.
Haffner, L. M. & David M. Meyer. (1995). A Search for Interstellar C 3 in the Translucent Cloud toward HD 147889. The Astrophysical Journal. 453. 450–450. 40 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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