Storm time empirical model of O+ and O6+ distributions in the magnetosphere-Reference-Cited by-同舟云学术

Storm time empirical model of O+ and O6+ distributions in the magnetosphere

Published:2017-08 Issue:8 Volume:122 Page:8353-8374
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Allen R. C.¹²^ORCID,Livi S. A.¹²^ORCID,Vines S. K.³^ORCID,Goldstein J.¹²^ORCID,Cohen I.³^ORCID,Fuselier S. A.¹²^ORCID,Mauk B. H.³^ORCID,Spence H. E.⁴^ORCID

Affiliation:

1. Space Science and Engineering Division; Southwest Research Institute; San Antonio Texas USA

2. Department of Physics and Astronomy; University of Texas at San Antonio; San Antonio Texas USA

3. Applied Physics Laboratory; The Johns Hopkins University; Laurel Maryland USA

4. Space Science Center; University of New Hampshire; Durham New Hampshire USA

Funder

Astrophysics Science Division

National Aeronautics and Space Administration

NASA Prime

JHU/APL

NASA/GSFC

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2017JA024245/fullpdf

Reference60 articles.

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2. Magnetic latitude dependence of oxygen charge states in the global magnetosphere: Insights into solar wind-originating ion injection;Allen;J. Geophys. Res. Space Physics,2016b

3. The Composition of Thermal and Hot Ions Observed by the GEOS-1 and -2 Spacecraft

4. Global ENA observations of the storm main phase ring current: Implications for skewed electric fields in the inner magnetosphere;Brandt;Geophys. Res. Lett.,2002

5. Magnetospheric Multiscale overview and science objectives;Burch;Space Sci. Rev.,2016

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