Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/38043
Title: Modeling the magnetospheric X-ray emission from solar wind charge exchange with verification from XMM-Newton observations
Authors: Whittaker, Ian C.
Sembay, Steve
Carter, Jennifer A.
Read, Andrew M.
Milan, Steve E.
Palmroth, Minna
First Published: 1-May-2016
Publisher: American Geophysical Union (AGU)
Citation: Journal of Geophysical Research: Space Physics, 2016, 121 (5), pp. 4158-4179
Abstract: An MHD-based model of terrestrial solar wind charge exchange (SWCX) is created and compared to 19 case study observations in the 0.5–0.7 keV emission band taken from the European Photon Imaging Cameras on board XMM-Newton. This model incorporates the Global Unified Magnetosphere-Ionosphere Coupling Simulation-4 MHD code and produces an X-ray emission datacube from O⁷⁺ and O⁸⁺ emission lines around the Earth using in situ solar wind parameters as the model input. This study details the modeling process and shows that fixing the oxygen abundances to a constant value reduces the variance when comparing to the observations, at the cost of a small accuracy decrease in some cases. Using the ACE oxygen data returns a wide ranging accuracy, providing excellent correlation in a few cases and poor/anticorrelation in others. The sources of error for any user wishing to simulate terrestrial SWCX using an MHD model are described here and include mask position, hydrogen to oxygen ratio in the solar wind, and charge state abundances. A dawn-dusk asymmetry is also found, similar to the results of empirical modeling. Using constant oxygen parameters, magnitudes approximately double that of the observed count rates are returned. A high accuracy is determined between the model and observations when comparing the count rate difference between enhanced SWCX and quiescent periods.
DOI Link: 10.1002/2015JA022292
ISSN: 2169-9380
eISSN: 2169-9402
Links: http://onlinelibrary.wiley.com/doi/10.1002/2015JA022292/abstract;jsessionid=7044E62E69CDEB5421A2C4AF2193AB81.f04t01
http://hdl.handle.net/2381/38043
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © the authors, 2016. This is an open-access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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