The average configuration of the induced Venus magnetotailThe interaction of the solar-wind flow with Venus is discussed as well as the morphology of magnetic-field-line draping in the Venus magnetotail. Emphasis is placed on the importance of the interplanetary magnetic field X-component in controlling the configuration of field draping in this induced magnetotail. The average magnetic configuration of this magnetotail is studied. A connection is made between the derived consistent plasma flow speed and density and the observational energy/charge range and sensitivity of the Pioneer Venus Orbiter plasma analyzer.
Document ID
19880059341
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Mccomas, D. J. (Los Alamos National Laboratory NM, United States)
Spence, H. E. (Los Alamos National Lab. NM, United States)
Russell, C. T. (California, University Los Angeles, United States)