Short wavelength electromagnetic perturbations excited near the Solar Probe Plus spacecraft in the inner heliosphere: 2.5D hybrid modeling
dc.contributor.author | Lipatov, Alexander | |
dc.contributor.author | Sittler Jr., Edward C. | |
dc.contributor.author | Hartle, Richard E. | |
dc.contributor.author | Cooper, John F. | |
dc.date.accessioned | 2024-01-29T10:22:00Z | |
dc.date.available | 2024-01-29T10:22:00Z | |
dc.date.issued | 2011-12-14 | |
dc.description.abstract | A 2.5D numerical plasma model of the interaction of the solar wind (SW) with the Solar Probe Plus spacecraft (SPPSC) is presented. These results should be interpreted as a basic plasma model derived from the SW interaction with the spacecraft (SC), which could have consequences for both plasma wave and electron plasma measurements on board the SC in the inner heliosphere. Compression waves and electric field jumps with amplitudes of about 1.5 V/m and (12-18) V/m were also observed. A strong polarization electric field was also observed in the wing of the plasma wake. However, 2.5D hybrid modeling did not show excitation of whistler/Alfvén waves in the upstream connected with the bi-directional current closure that was observed in short-time 3D modeling SPPSC and near a tether in the ionosphere. The observed strong electromagnetic perturbations may be a crucial point in the electromagnetic measurements planned for the future Solar Probe Plus (SPP) mission. The results of modeling electromagnetic field perturbations in the SW due to “shot” noise in absence of SPPSC are also discussed. | |
dc.description.sponsorship | E.C. Sittler and A.S. Lipatov were supported in part by NASA Grant no. 93672302010619 (PI—E.C. Sittler) through NASA GSFC and GPHI/GEST Center UMBC, respectively. Computational resources were provided by the NASA’s High-End Computing Center at NASA Goddard Center and Advanced Supercomputing Division at Ames Center through the NASA Computational Grants SMD-07-0458 and SMD-08-0636. | |
dc.description.uri | https://www.sciencedirect.com/science/article/abs/pii/S0032063311003527 | |
dc.format.extent | 8 pages | |
dc.genre | journal articles | |
dc.identifier.citation | Lipatov, Alexander S., Edward C. Sittler Jr., Richard E. Hartle, and John F. Cooper. “Short Wavelength Electromagnetic Perturbations Excited near the Solar Probe Plus Spacecraft in the Inner Heliosphere: 2.5D Hybrid Modeling.” Planetary and Space Science 62, no. 1 (March 1, 2012): 61–68. https://doi.org/10.1016/j.pss.2011.12.008. | |
dc.identifier.uri | https://doi.org/10.1016/j.pss.2011.12.008 | |
dc.identifier.uri | http://hdl.handle.net/11603/31496 | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Goddard Planetary Heliophysics Institute (GPHI) | |
dc.relation.ispartof | UMBC Faculty Collection | |
dc.relation.ispartof | UMBC GESTAR II | |
dc.rights | This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. | |
dc.rights | Public Domain Mark 1.0 | en |
dc.rights.uri | https://creativecommons.org/publicdomain/mark/1.0/ | |
dc.title | Short wavelength electromagnetic perturbations excited near the Solar Probe Plus spacecraft in the inner heliosphere: 2.5D hybrid modeling | |
dc.type | Text | |
dcterms.creator | https://orcid.org/0000-0001-5026-8214 |