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Flux Rope Modeling of the 2022 September 5 Coronal Mass Ejection Observed by Parker Solar Probe and Solar Orbiter from 0.07 to 0.69 au

Davies, Emma E., Rüdisser, Hannah T., Amerstorfer, Ute V., Möstl, Christian, Bauer, Maike, Weiler, Eva, Amerstorfer, Tanja, Majumdar, Satabdwa, Hess, Phillip, Weiss, Andreas J., Reiss, Martin A., Green, Lucie M., Long, David M. orcid logoORCID: 0000-0003-3137-0277, Nieves-Chinchilla, Teresa, Trotta, Domenico, Horbury, Timothy S., O'Brien, Helen, Fauchon-Jones, Edward, Morris, Jean, Owen, Christopher J., Bale, Stuart D. and Kasper, Justin C. (2024) Flux Rope Modeling of the 2022 September 5 Coronal Mass Ejection Observed by Parker Solar Probe and Solar Orbiter from 0.07 to 0.69 au. The Astrophysical Journal: an international review of astronomy and astronomical physics, 973 (1). p. 51. ISSN 1538-4357

Metadata
Item Type:Article (Published)
Refereed:Yes
Uncontrolled Keywords:Solar coronal mass ejections; Heliosphere; Dynamical evolution; Solar wind; Physics; Space Physics, Astrophysics
Subjects:Physical Sciences > Astronomy
Physical Sciences > Astronomy > Astrophysics
DCU Faculties and Centres:DCU Faculties and Schools > Faculty of Science and Health
DCU Faculties and Schools > Faculty of Science and Health > School of Physical Sciences
Publisher:Institute of Physics Publishing, Inc.
Official URL:https://iopscience.iop.org/article/10.3847/1538-43...
Copyright Information:Authors
ID Code:33392
Deposited On:28 Sep 2026 10:09 by David Long . Last Modified 28 Sep 2026 10:09
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