The Genesis Solar-Wind Collector Materials

被引：0

作者：

A.J.G. Jurewicz

D.S. Burnett

R.C. Wiens

T.A. Friedmann

C.C. Hays

R.J. Hohlfelder

K. Nishiizumi

J.A. Stone

D.S. Woolum

R. Becker

A.L. Butterworth

A.J. Campbell

M. Ebihara

I.A. Franchi

V. Heber

C.M. Hohenberg

M. Humayun

K.D. McKeegan

K. McNamara

A. Meshik

R.O. Pepin

D. Schlutter

R. Wieler

机构：

[1] Jet Propulsion Laboratory/California Institute of Technology,Dept. of Physics

[2] California Institute of Technology,Dept. of Chemistry

[3] Los Alamos National Laboratory,Dept. Of Physics

[4] Sandia National Labs,Dept. of Earth and Space Sciences

[5] Space Sciences Lab. U. Calif,undefined

[6] Calif. St. U,undefined

[7] Dept. of Physics,undefined

[8] U. Minnesota,undefined

[9] Planetary Science Research Institute,undefined

[10] Open U,undefined

[11] Dept. of Geophysical Sciences,undefined

[12] U. of Chicago,undefined

[13] Tokyo Metropolitan University,undefined

[14] Institute for Isotope Geology and Mineral Resources,undefined

[15] Washington U,undefined

[16] UCLA,undefined

[17] NASA Johnson Space Center,undefined

来源：

Space Science Reviews | 2003年 / 105卷

关键词：

Solar Wind; Sapphire; Bulk Metallic Glass; Solar Energetic Particle; Collector Material;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Genesis (NASA Discovery Mission #5) is a sample return mission. Collectors comprised of ultra-high purity materials will be exposed to the solar wind and then returned to Earth for laboratory analysis. There is a suite of fifteen types of ultra-pure materials distributed among several locations. Most of the materials are mounted on deployable panels (‘collector arrays’), with some as targets in the focal spot of an electrostatic mirror (the ‘concentrator’). Other materials are strategically placed on the spacecraft as additional targets of opportunity to maximize the area for solar-wind collection.

引用

页码：535 / 560

页数：25

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