Interstellar Boundary Explorer (IBEX)
Editat de David McComas, Gary Zank, Nathan Schwadronen Limba Engleză Paperback – 18 iun 2014
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Specificații
ISBN-13: 9781489999245
ISBN-10: 1489999248
Pagini: 380
Ilustrații: VII, 369 p.
Dimensiuni: 155 x 235 x 20 mm
Greutate: 0.53 kg
Ediția:2010
Editura: Springer
Colecția Springer
Locul publicării:New York, NY, United States
ISBN-10: 1489999248
Pagini: 380
Ilustrații: VII, 369 p.
Dimensiuni: 155 x 235 x 20 mm
Greutate: 0.53 kg
Ediția:2010
Editura: Springer
Colecția Springer
Locul publicării:New York, NY, United States
Public țintă
ResearchCuprins
Foreword.- Acknowledgements.- IBEX—Interstellar Boundary Explorer.- The IBEX Flight Segment.- The Interstellar Boundary Explorer High Energy (IBEX-Hi) Neutral Atom Imager.- The IBEX Background Monitor.- The IBEX-Lo Sensor.- Diagnosing the Neutral Interstellar Gas Flow at 1 AU with IBEX-Lo.- IBEX Backgrounds and Signal-to-Noise Ratio.- The Interstellar Boundary Explorer Science Operations Center.- The Galactic Environment of the Sun: Interstellar Material Inside and Outside of the Heliosphere.- Physical Processes in the Outer Heliosphere.- Physics of the Solar Wind–Local Interstellar Medium Interaction: Role of Magnetic Fields.- Kinetic-Gasdynamic Modeling of the Heliospheric Interface.- IBEX Education and Public Outreach.
Textul de pe ultima copertă
The Interstellar Boundary Explorer (IBEX) is a small explorer mission with the sole, focused science objective to discover the global interaction between the solar wind and the interstellar medium. IBEX is designed to achieve this objective by answering four fundamental science questions:
What is the global strength and structure of the termination shock?
How are energetic protons accelerated at the termination shock?
What are the global properties of the solar wind flow beyond the termination shock and in the heliotail?, and
How does the interstellar flow interact with the heliosphere beyond the heliopause?
The answers to these questions rely on IBEX’s energy resolved images of energetic neutral atoms (ENAs), which originate beyond the termination shock, in the inner heliosheath.
What is the global strength and structure of the termination shock?
How are energetic protons accelerated at the termination shock?
What are the global properties of the solar wind flow beyond the termination shock and in the heliotail?, and
How does the interstellar flow interact with the heliosphere beyond the heliopause?
The answers to these questions rely on IBEX’s energy resolved images of energetic neutral atoms (ENAs), which originate beyond the termination shock, in the inner heliosheath.
Caracteristici
Provides the basis for the interpretation of IBEX mission data Reveals the need for the unique data produced by IBEX Details the development of the elements of the IBEX flight system