INCA - THE ION-NEUTRAL CAMERA FOR ENERGETIC NEUTRAL ATOM IMAGING OF THE SATURNIAN MAGNETOSPHERE

被引:25
|
作者
MITCHELL, DG
CHENG, AF
KRIMIGIS, SM
KEATH, EP
JASKULEK, SE
MAUK, BH
MCENTIRE, RW
ROELOF, EC
WILLIAMS, DJ
HSIEH, KC
DRAKE, VA
机构
[1] UNIV ARIZONA, DEPT PHYS, LUNAR & PLANETARY LAB, TUCSON, AZ 85721 USA
[2] JOHNS HOPKINS UNIV, DEPT SPACE, APPL PHYS LAB, LAUREL, MD 20723 USA
[3] JOHNS HOPKINS UNIV, APPL PHYS LAB, MAGNETOSPHER PARTICLE PHYS SECT, LAUREL, MD 20723 USA
[4] JOHNS HOPKINS UNIV, MILTON S EISENHOWER RES CTR, APPL PHYS LAB, LAUREL, MD 20723 USA
关键词
MAGNETOSPHERIC IMAGERY; ATMOSPHERIC REMOTE SENSING; ENERGETIC NEUTRAL ATOMS; MICROCHANNEL PLATES; MAGNETOSPHERIC ION COMPOSITION; THIN FOILS; SECONDARY ELECTRON YIELD;
D O I
10.1117/12.155609
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Techniques developed for the detection and characterization of energetic (>20 keV) ions in space plasmas have been modified to include imaging so that energetic neutral atoms at Saturn may be used to form images of the Saturnian magnetosphere and its interaction with the atmosphere of the moon Titan. The basic elements of the ion-neutral camera head on the magnetospheric imaging instrument for the Cassini mission are described, with emphasis on developmental detection techniques and components. In particular, pulse-height analysis of the microchannel plate responses to different mass neutrals is used for rough composition determination, and deflection plates in the aperture as well as time-of-flight measurements allow imaging of neutral atoms from within regions of moderate intensity ambient ion and electron fluxes.
引用
收藏
页码:3096 / 3101
页数:6
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