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The Interstellar Boundary Explorer (IBEX)

 

作者: David McComas,   Frederic Allegrini,   Peter Bochsler,   Maciej Bzowski,   Michael Collier,   Hans Fahr,   Horst Fichtner,   Priscilla Frisch,   Herb Funsten,   Steve Fuselier,   George Gloeckler,   Mike Gruntman,   Vlad Izmodenov,   Paul Knappenberger,   Marty Lee,   Stefano Livi,   Don Mitchell,   Eberhard Mo¨bius,   Tom Moore,   Dan Reisenfeld,   Ed Roelof,   Nathan Schwadron,   Martin Wieser,   Manfred Witte,   Peter Wurz,   Gary Zank,  

 

期刊: AIP Conference Proceedings  (AIP Available online 1904)
卷期: Volume 719, issue 1  

页码: 162-181

 

ISSN:0094-243X

 

年代: 1904

 

DOI:10.1063/1.1809514

 

出版商: AIP

 

数据来源: AIP

 

摘要:

The Interstellar Boundary Explorer (IBEX) is one of five Small Explorer (SMEX) missions undergoing Phase A study for NASA’s Office of Space Science. Around November 2004, NASA expects to select at least one of missions for development and flight. If selected, IBEX will provide the first global views of the Sun’s interstellar boundaries by taking a set of global energetic neutral atom (ENA) images at a variety of energies. Recent advances in ENA imaging have made it possible to remotely image space plasmas and ENA imaging is now poised to image the interstellar interactions and interstellar boundaries at the edge of our heliosphere. IBEX makes these exploratory ENA observations using two ultra‐high sensitivity ENA cameras on a simple spinning spacecraft. IBEX’s highly elliptical Earth orbit allows viewing of the outer heliosphere from beyond the Earth’s relatively bright magnetospheric ENA emissions. IBEX’s sole, focused science objective is to discover the global interaction between the solar wind and the interstellar medium. IBEX achieves this objective by answering four fundamental science questions: (1) What is the global strength and structure of the termination shock? (2) How are energetic protons accelerated at the termination shock? (3) What are the global properties of the solar wind flow beyond the termination shock and in the heliotail? and (4) How does the interstellar flow interact with the heliosphere beyond the heliopause? The IBEX objective is central to the Sun‐Earth Connection (SEC) theme as demonstrated by both the 2003 SEC Roadmap and 2002 NRC’s Decadal Survey and is specifically identified in the 2003 NASA‐wide Strategic Plan. In short, the IBEX mission provides the first global views of the Sun’s interstellar boundaries, unveiling the physics of the heliosphere’s interstellar interaction, providing a deeper understanding of the heliosphere and thereby astrospheres throughout the galaxy, and creating the opportunity to make even greater unanticipated discoveries. © 2004 American Institute of Physics

 

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