A comparative study of distant magnetotail structure at Venus and Earth
Authors:
- J. A. SlavinJSJ. A. Slavin
- E. J. SmithESE. J. Smith
- D. S. IntriligatorDID. S. Intriligator
Open Access
- 1 October 1984
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 11 (10) , 1074-1077
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- Wave‐particle interactions in the Venus wake and tailJournal of Geophysical Research, 1984
- Magnetic structure of the distant geotail from −60 to −220 Re: ISEE‐3Geophysical Research Letters, 1984
- Average configuration of the distant (e) magnetotail: Initial ISEE‐3 magnetic field resultsGeophysical Research Letters, 1983
- Plasma regimes in the deep geomagnetic tail: ISEE 3Geophysical Research Letters, 1983
- The viscous-like magnetospheric convection and the length of the earth's magnetotailPlanetary and Space Science, 1983
- Venus nightside ionospheric holes: The signatures of parallel electric field acceleration regions?Geophysical Research Letters, 1981
- The distant bow shock and magnetotail of Venus: Magnetic field and plasma wave observationsGeophysical Research Letters, 1981
- Viscous Flow Circulation of the Solar Wind Behind VenusScience, 1980