Journal article
Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe
Space science reviews, Vol.219(2), pp.18-18
03/01/2023
DOI: 10.1007/s11214-022-00943-x
PMCID: PMC9974711
PMID: 36874191
Abstract
A detailed overview of the knowledge gaps in our understanding of the heliospheric interaction with the largely unexplored Very Local Interstellar Medium (VLISM) are provided along with predictions of with the scientific discoveries that await. The new measurements required to make progress in this expanding frontier of space physics are discussed and include in-situ plasma and pick-up ion measurements throughout the heliosheath, direct sampling of the VLISM properties such as elemental and isotopic composition, densities, flows, and temperatures of neutral gas, dust and plasma, and remote energetic neutral atom (ENA) and Lyman-alpha (LYA) imaging from vantage points that can uniquely discern the heliospheric shape and bring new information on the interaction with interstellar hydrogen. The implementation of a pragmatic Interstellar Probe mission with a nominal design life to reach 375 Astronomical Units (au) with likely operation out to 550 au are reported as a result of a 4-year NASA funded mission study.
Details
- Title: Subtitle
- Future Exploration of the Outer Heliosphere and Very Local Interstellar Medium by Interstellar Probe
- Creators
- P. C. Brandt - Johns Hopkins University Applied Physics LaboratoryE. Provornikova - Johns Hopkins University Applied Physics LaboratoryS. D. Bale - University of California, BerkeleyA. Cocoros - Johns Hopkins University Applied Physics LaboratoryR. DeMajistre - Johns Hopkins University Applied Physics LaboratoryK. Dialynas - Academy of AthensH. A. Elliott - Southwest Research InstituteS. Eriksson - Laboratory for Atmospheric and Space PhysicsB. Fields - University of Illinois Urbana-ChampaignA. Galli - University of BernM. E. Hill - Johns Hopkins University Applied Physics LaboratoryM. Horanyi - Laboratory for Atmospheric and Space PhysicsT. Horbury - Imperial College LondonS. Hunziker - ETH ZurichP. Kollmann - Johns Hopkins University Applied Physics LaboratoryJ. Kinnison - Johns Hopkins University Applied Physics LaboratoryG. Fountain - Johns Hopkins University Applied Physics LaboratoryS. M. Krimigis - Academy of AthensW. S. Kurth - University of IowaJ. Linsky - University of Colorado BoulderC. M. Lisse - Johns Hopkins University Applied Physics LaboratoryK. E. Mandt - Johns Hopkins University Applied Physics LaboratoryW. Magnes - Austrian Academy of SciencesR. L. McNutt - Johns Hopkins University Applied Physics LaboratoryJ. Miller - Boston UniversityE. Moebius - University of New HampshireP. Mostafavi - Johns Hopkins University Applied Physics LaboratoryM. Opher - Boston UniversityL. Paxton - Johns Hopkins University Applied Physics LaboratoryF. Plaschke - Technische Universität BraunschweigA. R. Poppe - University of California, BerkeleyE. C. Roelof - Johns Hopkins University Applied Physics LaboratoryK. Runyon - Planetary Science InstituteS. Redfield - Laurel UniversityN. Schwadron - University of New Hampshire at ManchesterV. Sterken - ETH ZurichP. Swaczyna - Princeton UniversityJ. Szalay - Princeton UniversityD. Turner - Johns Hopkins University Applied Physics LaboratoryH. Vannier - Laurel UniversityR. Wimmer-Schweingruber - Christian-Albrechts-Universität zu KielP. Wurz - University of BernE. J. Zirnstein - Princeton University
- Resource Type
- Journal article
- Publication Details
- Space science reviews, Vol.219(2), pp.18-18
- DOI
- 10.1007/s11214-022-00943-x
- PMID
- 36874191
- PMCID
- PMC9974711
- NLM abbreviation
- Space Sci Rev
- ISSN
- 0038-6308
- eISSN
- 1572-9672
- Publisher
- Springer Netherlands
- Grant note
- ; NNN06AA01C / ; NAS5 97271; NNX07AJ69G; NNN06AA01C; 80NSSC20K0719; 80GSFC19C0027 / ;
- Language
- English
- Date published
- 03/01/2023
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984455551102771
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