The Cassini Magnetic Field Investigation

被引:1
|
作者
M. K. Dougherty
S. Kellock
D. J. Southwood
A. Balogh
E. J. Smith
B. T. Tsurutani
B. Gerlach
K.-H. Glassmeier
F. Gleim
C. T. Russell
G. Erdos
F. M. Neubauer
S. W. H. Cowley
机构
[1] Imperial College,The Blackett Laboratory
[2] California Institute of Technology,Jet Propulsion Laboratory
[3] Technische Universitat Braunschweig,Institute for Geophysics and Meterology
[4] UCLA Institute of Geophysics and Planetary Physics,Department of Physics and Astronomy
[5] KFKI Research Institute for Particle and Nuclear Physics,undefined
[6] Köln University,undefined
[7] Leicester University,undefined
来源
Space Science Reviews | 2004年 / 114卷
关键词
Cassini; magnetometer; saturn;
D O I
暂无
中图分类号
学科分类号
摘要
The dual technique magnetometer system onboard the Cassini orbiter is described. This instrument consists of vector helium and fluxgate magnetometers with the capability to operate the helium device in a scalar mode. This special mode is used near the planet in order to determine with very high accuracy the interior field of the planet. The orbital mission will lead to a detailed understanding of the Saturn/Titan system including measurements of the planetary magnetosphere, and the interactions of Saturn with the solar wind, of Titan with its environments, and of the icy satellites within the magnetosphere.
引用
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页码:331 / 383
页数:52
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