Summary of interplanetary and interstellar dust observation by Mars Dust Counter on board NOZOMI

被引：7
|
作者：
Sasaki, S. [1 ]
Igenbergs, E. [2 ]
Ohashi, H. [3 ,5 ]
Senger, R. [2 ]
Muenzenmayer, R. [4 ]
Naumann, W.
Grun, E. [6 ]
Nogami, K. [7 ]
Mann, I. [8 ]
Svedhem, H. [8 ]
机构：
[1] Natl Inst Nat Sci, Natl Astron Observ Japan, RISE Project Off, Oshu, Iwate 0230861, Japan
[2] Tech Univ Munich, LRT, D-85748 Garching, Germany
[3] Tokyo Univ Marine Sci & Technol, Minato Ku, Tokyo 1080075, Japan
[4] Astrium Space, D-88039 Friedrichshafen, Germany
[5] Kayser Threde GmbH, D-81379 Munich, Germany
[6] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany
[7] Dokkyo Univ, Sch Med, Mibu, Tochigi 3120207, Japan
[8] European Space Agcy, Estec, Dept Space Sci, NL-2200 AG Noordwijk, Netherlands
来源：
ADVANCES IN SPACE RESEARCH | 2007年 / 39卷 / 03期
关键词：
interplanetary dust; interstellar dust; dust detector; meteor stream; circumterrestrial dust; NOZOMI;
D O I：
10.1016/j.asr.2006.11.006
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Mars Dust Counter (MDC) is a light-weight dust detector of impact ionization type on board Japanese Mars mission NOZOMI. NOZOMI was launched on July 4th (3rd at UT) 1998. From December 1998 to December 2003 for five years, NOZOMI took eccentric orbits between the Earth's and Mars' orbits. Until April 2002, MDC continuously observed interplanetary dust. MDC has detected nearly 100 doubtless dust impacts. There were observed several high-velocity particles, which are apparently different from Keplerian dust particles gravitationally bound to the sun. Directional analysis showed that MDC has detected several particles of interstellar origin during the cruising phase of NOZOMI. (C) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码：485 / 488
页数：4
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