Composition of hot ions (0.1–16 keV/e) as observed by the geoos and ISEE mass spectrometers and inferences for the origin and circulation of magnetospheric plasmas-Reference-Cited by-同舟云学术

Composition of hot ions (0.1–16 keV/e) as observed by the geoos and ISEE mass spectrometers and inferences for the origin and circulation of magnetospheric plasmas

Published:1981-01 Issue:1 Volume:1 Page:289-303
ISSN:0273-1177
Container-title:Advances in Space Research
language:en
Short-container-title:Advances in Space Research

Author:

Balsiger H.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference19 articles.

1. Magnetic storm injection of 0.9- to 16-keV/e solar and terrestrial ions into the high-altitude magnetosphere

2. Heavy ions in the magnetosphere

3. Quantitative Modelling of Magnetospheric Processes;Young,1979

4. Energetic ion composition in the Earth's magnetosphere

5. Some initial ISEE-1 results on the ring current composition and dynamics during the magnetic storm of December 11, 1977

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