D. K. Haggerty

4.4k total citations
93 papers, 2.4k citations indexed

About

D. K. Haggerty is a scholar working on Astronomy and Astrophysics, Molecular Biology and Artificial Intelligence. According to data from OpenAlex, D. K. Haggerty has authored 93 papers receiving a total of 2.4k indexed citations (citations by other indexed papers that have themselves been cited), including 83 papers in Astronomy and Astrophysics, 16 papers in Molecular Biology and 8 papers in Artificial Intelligence. Recurrent topics in D. K. Haggerty's work include Solar and Space Plasma Dynamics (67 papers), Astro and Planetary Science (63 papers) and Ionosphere and magnetosphere dynamics (53 papers). D. K. Haggerty is often cited by papers focused on Solar and Space Plasma Dynamics (67 papers), Astro and Planetary Science (63 papers) and Ionosphere and magnetosphere dynamics (53 papers). D. K. Haggerty collaborates with scholars based in United States, Germany and United Kingdom. D. K. Haggerty's co-authors include E. C. Roelof, G. M. Mason, C. M. S. Cohen, C. Paranicas, R. A. Mewaldt, B. H. Mauk, P. Kollmann, R. A. Leske, M. D. Looper and G. M. Simnett and has published in prestigious journals such as Nature, Science and Journal of Geophysical Research Atmospheres.

In The Last Decade

D. K. Haggerty

88 papers receiving 2.3k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
D. K. Haggerty United States 25 2.3k 490 134 126 88 93 2.4k
S. Akiyama United States 26 2.4k 1.0× 502 1.0× 198 1.5× 96 0.8× 119 1.4× 82 2.4k
Nicole Vilmer France 25 2.0k 0.8× 319 0.7× 147 1.1× 247 2.0× 129 1.5× 99 2.0k
Daikou Shiota Japan 24 1.7k 0.7× 451 0.9× 149 1.1× 80 0.6× 111 1.3× 65 1.7k
D. Lario United States 28 3.2k 1.4× 367 0.7× 364 2.7× 234 1.9× 86 1.0× 149 3.3k
R. B. McKibben United States 25 1.8k 0.8× 358 0.7× 153 1.1× 186 1.5× 37 0.4× 92 1.9k
Noé Lugaz United States 35 3.3k 1.4× 966 2.0× 160 1.2× 51 0.4× 126 1.4× 140 3.4k
S. Freeland United States 11 1.9k 0.8× 356 0.7× 188 1.4× 81 0.6× 41 0.5× 14 2.0k
K.‐P. Wenzel Netherlands 16 1.4k 0.6× 329 0.7× 77 0.6× 252 2.0× 115 1.3× 64 1.5k
N. Nitta United States 34 4.2k 1.8× 1.0k 2.1× 265 2.0× 156 1.2× 179 2.0× 163 4.2k
A. Lara Mexico 24 2.2k 1.0× 519 1.1× 130 1.0× 78 0.6× 104 1.2× 82 2.4k

Countries citing papers authored by D. K. Haggerty

Since Specialization
Citations

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

Fields of papers citing papers by D. K. Haggerty

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by D. K. Haggerty. 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 D. K. Haggerty. The network helps show where D. K. Haggerty may publish in the future.

Co-authorship network of co-authors of D. K. Haggerty

This figure shows the co-authorship network connecting the top 25 collaborators of D. K. Haggerty. A scholar is included among the top collaborators of D. K. Haggerty 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 D. K. Haggerty. D. K. Haggerty 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.
Mauk, B. H., Qianli Ma, Heidi N. Becker, et al.. (2024). Upward, MeV‐Class Electron Beams Over Jupiter's Main Aurora. Geophysical Research Letters. 51(24). 3 indexed citations
2.
Nichols, J. D., F. Allegrini, F. Bagenal, et al.. (2023). Jovian Magnetospheric Injections Observed by the Hubble Space Telescope and Juno. Geophysical Research Letters. 50(20). 6 indexed citations
3.
Mauk, B. H., J. R. Szalay, F. Allegrini, et al.. (2023). How Bi‐Modal Are Jupiter's Main Aurora Zones?. Journal of Geophysical Research Space Physics. 128(4). 8 indexed citations
4.
Kollmann, P., G. Clark, C. Paranicas, et al.. (2022). Ganymede's Radiation Cavity and Radiation Belts. Geophysical Research Letters. 49(23). 6 indexed citations
5.
Kollmann, P., G. Clark, C. Paranicas, et al.. (2021). Jupiter's Ion Radiation Belts Inward of Europa's Orbit. Journal of Geophysical Research Space Physics. 126(4). 11 indexed citations
6.
Mauk, B. H., F. Allegrini, F. Bagenal, et al.. (2020). Energetic Neutral Atoms From Jupiter's Polar Regions. Journal of Geophysical Research Space Physics. 125(12). 5 indexed citations
7.
Mauk, B. H., G. Clark, G. R. Gladstone, et al.. (2020). Energetic Particles and Acceleration Regions Over Jupiter's Polar Cap and Main Aurora: A Broad Overview. Journal of Geophysical Research Space Physics. 125(3). 60 indexed citations
8.
Haggerty, D. K., B. H. Mauk, C. Paranicas, et al.. (2019). Jovian Injections Observed at High Latitude. Geophysical Research Letters. 46(16). 9397–9404. 23 indexed citations
9.
Kollmann, P., B. H. Mauk, G. Clark, et al.. (2019). Jupiter's Innermost Radiation Belts from Juno Measurements. AGU Fall Meeting Abstracts. 2019. 1 indexed citations
10.
Mauk, B. H., D. K. Haggerty, C. Paranicas, et al.. (2018). Diverse Electron and Ion Acceleration Characteristics Observed Over Jupiter's Main Aurora. Geophysical Research Letters. 45(3). 1277–1285. 56 indexed citations
11.
Paranicas, C., B. H. Mauk, D. K. Haggerty, et al.. (2018). Intervals of Intense Energetic Electron Beams Over Jupiter's Poles. Journal of Geophysical Research Space Physics. 123(3). 1989–1999. 33 indexed citations
12.
Kollmann, P., C. Paranicas, G. Clark, et al.. (2017). A heavy ion and proton radiation belt inside of Jupiter's rings. Geophysical Research Letters. 44(11). 5259–5268. 26 indexed citations
13.
Cohen, C. M. S., M. E. Wiedenbeck, G. M. Mason, et al.. (2013). Furthering Our Understanding of Wide Longitude 3He-rich SEP Events. ICRC. 33. 1420. 1 indexed citations
14.
Gómez‐Herrero, R., R. Mueller‐Mellin, A. Klassen, et al.. (2008). Simultaneous ACE/STEREO Observations of Solar Electron Events in May 2007. 37. 749. 2 indexed citations
15.
Livi, S., G. C. Ho, & D. K. Haggerty. (2006). A Novel - very High Sensitivity Mass Spectrometer for Planetary Atmospheres Measurements. 36. 2076. 1 indexed citations
16.
Mewaldt, R. A., C. M. S. Cohen, R. A. Leske, et al.. (2005). Solar Energetic Particle Composition, Energy Spectra and Timing in the January 20, 2005 Event. AGUFM. 2005.
17.
Simnett, G. M., E. C. Roelof, & D. K. Haggerty. (2004). The Source of Short (<1 hour) Beams of Near-relativistic Electrons Seen by ACE. AGU Spring Meeting Abstracts. 2004. 1 indexed citations
18.
Haggerty, D. K. & E. C. Roelof. (2002). Near-Relativistic Beam-Like Electron Events Observed at 1 AU. AGU Spring Meeting Abstracts. 2002.
19.
Simnett, G. M., E. C. Roelof, & D. K. Haggerty. (2001). What Have Impulsive Near-Relativistic Electron Events to do With CMEs?. AGU Spring Meeting Abstracts. 2001. 1 indexed citations
20.
Simnett, G. M., E. C. Roelof, & D. K. Haggerty. (2001). The Acceleration and Release of Near-Relativistic Electrons by CMEs. AGUFM. 2001. 4 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

Rankless by CCL
2026