Constraining the IMF at Pluto Using New Horizons SWAP Data and Hybrid Simulations-Reference-Cited by-同舟云学术

Constraining the IMF at Pluto Using New Horizons SWAP Data and Hybrid Simulations

Published:2019-03 Issue:3 Volume:124 Page:1568-1581
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Barnes N. P.¹^ORCID,Delamere P. A.¹^ORCID,Strobel D. F.²^ORCID,Bagenal F.³^ORCID,McComas D. J.⁴⁵^ORCID,Elliott H. A.⁵^ORCID,Valek P.⁵^ORCID,Weaver H. A.⁶^ORCID,Ennico K.⁷^ORCID,Young L. A.⁸^ORCID,Stern S. A.⁸^ORCID

Affiliation:

1. Geophysical Institute University of Alaska Fairbanks Fairbanks AK USA

2. Department of Earth and Planetary Sciences Johns Hopkins University Laurel MD USA

3. Laboratory for Atmospheric and Space Physics University of Colorado Boulder CO USA

4. Department of Astrophysical Sciences Princeton University Princeton NJ

5. Southwest Research Institute San Antonio TX USA

6. Johns Hopkins University Applied Physics Laboratory Johns Hopkins University Laurel MD USA

7. NASA Ames Research Center, Moffett Field CA USA

8. Southwest Research Institute Boulder CO USA

Funder

National Aeronautics and Space Administration

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2018JA026083

Reference43 articles.

1. The Uranian bow shock: Voyager 2 inbound observations of a high Mach number shock

2. Solar wind at 33 AU: Setting bounds on the Pluto interaction for New Horizons

3. Pluto’s interaction with its space environment: Solar wind, energetic particles, and dust

4. Pluto‧s interaction with the solar wind

5. Absolute detection efficiencies of a microchannel plate detector for ions

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