Journal article
Jupiter’s radiation belts as a target for NASA’s Heliophysics Division
Bulletin of the American Astronomical Society, Vol.55(3)
07/31/2023
DOI: 10.3847/25c2cfeb.6eb85c6e
Abstract
Jupiter is the largest particle accelerator in the solar system and therefore an ideal laboratory to study fundamental heliophysics.
Details
- Title: Subtitle
- Jupiter’s radiation belts as a target for NASA’s Heliophysics Division
- Creators
- P. Kollmann - Allentown Public LibraryO. Allanson - University of ExeterL. Arruda - LIP - Laboratory of Instrumentation and Experimental Particle PhysicsG. Berland - Laboratory for Atmospheric and Space PhysicsL. W. Blum - Laboratory for Atmospheric and Space PhysicsJ. Bortnik - NOAA Oceanic and Atmospheric ResearchX. Cao - Laboratory for Atmospheric and Space PhysicsT. Y. ChenG. Clark - Johns Hopkins University Applied Physics LaboratoryI. Cohen - Allentown Public LibraryJ. F. Cooper - NASA GSFC, Greenbelt MD, USA (Emeritus, Code 672)F. Crary - Laboratory for Atmospheric and Space PhysicsR. T. Desai - Imperial College LondonK. Dialynas - Academy of AthensA. Drozdov - Earth and Space ResearchO. V. Dudnik - National Academy of Sciences of UkraineW. R. Dunn - UCL, UKG. B. Hospodarsky - University of IowaH. Huybrighs - Khalifa University of Science and TechnologyA. N. Jaynes - University of IowaC. M. Jackman - Dublin Institute For Advanced StudiesI. Jun - NASA/JPL, Pasadena, CA, USAK. K. Khurana - Earth and Space ResearchR. Kraft - IIT@HarvardE. A. Kronberg - Ludwig-Maximilians-Universität MünchenS. Lejosne - University of California, BerkeleyW. Li - Boston UniversityX. Li - Laboratory for Atmospheric and Space PhysicsL. Liuzzo - University of California, BerkeleyQ. Ma - Boston UniversityR. Marshall - University of Colorado BoulderB. Mauk - Johns Hopkins University Applied Physics LaboratoryQ. Nénon - Institut de Recherche en Astrophysique et PlanétologieT. A. Nordheim - Space Information Laboratories (United States)C. Paranicas - Johns Hopkins University Applied Physics LaboratoryC. C. Plainaki - Agenzia Spaziale ItalianaL. H. Regoli - Johns Hopkins University Applied Physics LaboratoryE. Roussos - Max Planck Institute for Solar System ResearchY. Shprits - Leibniz Institute for Astrophysics PotsdamA. Siecard - Office National d'Études et de Recherches AérospatialesS. Simon - Georgia Institute of TechnologyH. T. Smith - Johns Hopkins University Applied Physics LaboratoryK. Sorathia - Johns Hopkins University Applied Physics LaboratoryH. E. Spence - University of New Hampshire at ManchesterA. Sulaiman - University of New Hampshire at ManchesterY. Sun - Peking Uni., Beijing, ChinaW. Tu - West Virginia UniversityD. L. Turner - Johns Hopkins University Applied Physics LaboratoryM. E. Usanova - Laboratory for Atmospheric and Space PhysicsP. Williams - IIT@HarvardE. E. Woodfield - BAS, Cambridge, UKX. Wu - DPNC, Uni. Geneva, SwitzerlandC.-J. Yuan - Institute of Geology and Geophysics
- Resource Type
- Journal article
- Publication Details
- Bulletin of the American Astronomical Society, Vol.55(3)
- DOI
- 10.3847/25c2cfeb.6eb85c6e
- ISSN
- 0002-7537
- eISSN
- 2330-9458
- Language
- English
- Date published
- 07/31/2023
- Academic Unit
- Physics and Astronomy; University College Courses
- Record Identifier
- 9984464481202771
Metrics
34 Record Views