The Chandra X-Ray Observatory: An overview

被引:29
作者
Weisskopf, MC [1 ]
机构
[1] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
来源
MAGNETIC HELICITY AT THE SUN, IN SOLAR WIND AND MAGNETOSPHERES: VISTAS FROM X-RAY OBSERVATORIES | 2003年 / 32卷 / 10期
关键词
D O I
10.1016/S0273-1177(03)90639-9
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Chandra X-Ray Observatory, one of NASA's Great Observatories, was successfully launched on July 23, 1999 by the Space Shuttle Columbia. After release from Columbia, an Inertial Upper Stage was used to further boost the observatory. After five subsequent firings over 15 days of an internal propulsion system, the Observatory was placed in a highly elliptical orbit. The first x-rays focussed by the telescope were observed on August 12, 1999. Despite an initial surprise that the x-ray telescope was far more efficient for concentrating low-energy protons than had been anticipated, the observatory is performing well and is returning superb scientific data. Operating together with other space observatories, most notably the recently activated XMM-Newton, it is clear that with Chandra we are entering a new era of discovery in high-energy astrophysics. Published by Elsevier Ltd on behalf of COSPAR.
引用
收藏
页码:2005 / 2011
页数:7
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