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The Living with a Star Radiation Belt Storm ProbesThe goal of NASA's Living With a Star Radiation Belt Storm Probe mission is to understand, ideally to the point of predictability, how populations of relativistic electrons and ions in space form or change in response to the variable inputs of energy from the Sun. The investigations selected for this 2-spacecraft mission scheduled for launch in early 2012 address this task by making extensive observations of the plasma waves, thermal, ring current, and relativistic particle populations, and DC electric and magnetic fields within the Earth's inner and outer radiation belts. We first describe the current mission concept within the scope of NASA's strategic plan and the Vision for Exploration, and then consider how its observations will be used to define and quantify the processes that accelerate, transport, and remove particles in the Earth's radiation belts.
Document ID
20070035742
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Sibeck, D. G.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Mauk, B. H.
(Johns Hopkins Univ. Laurel, MD, United States)
Grebowsky, J. M.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Fox, N. J.
(Johns Hopkins Univ. Laurel, MD, United States)
Date Acquired
August 24, 2013
Publication Date
March 9, 2007
Subject Category
Astronomy
Meeting Information
Meeting: LW Geostrom CDAW and Conference
Location: Melbourne, FL
Country: United States
Start Date: March 5, 2007
End Date: March 9, 2007
Distribution Limits
Public
Copyright
Other

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