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The Earth's Exosphere and Its Response to Space WeatherNeutral-Plasma charge exchange is a fundamental physical process that occurs ubiquitously across the universe. In geospace, charge exchange occurs in the Earth’s topside ionosphere, polar wind, plasmasphere, inner magnetosphere, and magnetosheath. Past and current space missions have profiled plasma and electromagnetic characteristics in various parts of the Earth’s magnetospheric system. However, observations of the exosphere, i.e., neutrals above 500 km altitude, are still sparse and, in some regions, non-existent, which limits our understanding of the neutral contribution to the overall dynamics of the geospace environment.
Cold exospheric neutrals (< 10 eV) play an important role in the Sun-Earth interaction. Variability of exospheric density provides key information of the Earth’s atmospheric loss under dynamic space environment conditions. Various neutral species and their density variations in the polar wind can alter ion outflow patterns, modifying global magnetospheric dynamics. Exospheric neutrals also provide an energy sink for the inner magnetosphere by creating Energetic Neutral Atoms (ENAs) through charge exchange with high-energy ring current ions, which subsequently leave our geospace system unimpeded by magnetic fields. Exospheric neutrals also provide a means to observe the global interaction of the solar wind – magnetosphere, through global imaging of the system via ENAs (e.g., the TWINS and IMAGE missions) and soft X-rays (e.g., the upcoming LEXI and SMILE missions), the byproducts of neutral-plasma charge exchange.
In the coming decade, we advocate that our community needs to increase our exploration of the neutral populations in the outermost reaches of the Earth’s atmosphere. It is imperative that we improve both in-situ and remote-sensing technologies for measuring key neutral species in our exosphere. We also encourage dedicated exosphere missions and to stimulate model developments of our exosphere and its interaction with the co-located magnetospheric system and neighboring Ionosphere - Thermosphere - Mesosphere system.
Document ID
20220016573
Acquisition Source
Goddard Space Flight Center
Document Type
White Paper
Authors
Hyunju Connor
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Dolon Bhattacharyya
(Laboratory for Atmospheric and Space Physics Boulder, Colorado, United States)
Seth Claudepierre
(University of California, Los Angeles Los Angeles, California, United States)
Gonzalo Cucho-Padin
(Catholic University of America Washington D.C., District of Columbia, United States)
Jaewoong Jung
(University of Alaska Fairbanks Fairbanks, Alaska, United States)
Dayeh Maher
(Southwest Research Institute San Antonio, Texas, United States)
Edwin Mierkiewicz
(Embry–Riddle Aeronautical University Daytona Beach, Florida, United States)
Susan Nossal
(University of Wisconsin–Madison Madison, Wisconsin, United States)
Kevin Pham
(National Center for Atmospheric Research Boulder, Colorado, United States)
Eric Sutton
(University of Colorado Boulder Boulder, Colorado, United States)
Yongliang Zhang
(Johns Hopkins University Applied Physics Laboratory North Laurel, Maryland, United States)
Date Acquired
November 2, 2022
Publication Date
December 31, 2022
Publication Information
Subject Category
Space Sciences (General)
Funding Number(s)
WBS: 364688.05.18.07.02
WBS: 981698.01.04.51.05.60.85
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
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