This three year study is concerned with theoretical aspects of basic solar wind properties and their effects on cosmic rays. Such studies are important analyzing the influence of highly energetic particles transmitted through the interplanetary medium on the terrestrial environment. The investigation will include studies of the large scale morphology of the interplanetary magnetic field and plasma, with particular emphasis on the effect of the field's structure on cosmic ray and energetic particle acceleration, propagation and anisotropies. ***//

Agency
National Science Foundation (NSF)
Institute
Division of Atmospheric and Geospace Sciences (AGS)
Application #
8922151
Program Officer
Kenneth H. Schatten
Project Start
Project End
Budget Start
1990-05-01
Budget End
1993-10-31
Support Year
Fiscal Year
1989
Total Cost
$251,800
Indirect Cost
Name
University of Arizona
Department
Type
DUNS #
City
Tucson
State
AZ
Country
United States
Zip Code
85721