A scenario for solar wind penetration of Earth's magnetic tail based on ion composition data from the ISEE 1 spacecraft
- 1 December 1992
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 97 (A12) , 19221-19238
- https://doi.org/10.1029/92ja01604
Abstract
No abstract availableKeywords
This publication has 44 references indexed in Scilit:
- Tail Plasma Domains and the Auroral Oval-Results of Mapping Based on the Tsyganenko 1989 Magnetosphere Model.Journal of geomagnetism and geoelectricity, 1992
- Plasma sheet ion composition at various levels of geomagnetic and solar activityPhysica Scripta, 1987
- A statistical study of the central plasma sheet: Implications for substorm modelsGeophysical Research Letters, 1986
- Magnetic structure of the distant geotail from −60 to −220 Re: ISEE‐3Geophysical Research Letters, 1984
- Helium abundance variations in the solar windSolar Physics, 1983
- The plasma mantle: Composition and other characteristics observed by means of the PROGNOZ-7 satelliteSpace Science Reviews, 1982
- Plasma populations in a simple open model magnetosphereSpace Science Reviews, 1980
- Plasma Flow in the Magnetotail and its Implications for Substorm TheoriesPublished by Springer Nature ,1979
- A Model of the Geomagnetic CavityRadio Science, 1971
- A UNIFYING THEORY OF HIGH-LATITUDE GEOPHYSICAL PHENOMENA AND GEOMAGNETIC STORMSCanadian Journal of Physics, 1961