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Mshpy23: A User-Friendly, Parameterized Model of Magnetosheath ConditionsLunar Environment heliospheric X-ray Imager (LEXI) and Solar wind – Magnetosphere - Ionosphere Link Explorer (SMILE) will observe magnetosheath and its boundary motion in soft X-rays for understanding magnetopause reconnection modes under varioussolar wind conditions after their respective launches in 2024 and 2025. Magnetosheath conditions, namely, plasma density, velocity, and temperature, are key parameters for predicting and analyzing soft X-ray images from the LEXI and SMILE missions. We developed a user-friendly model of magnetosheath that parameterizes number density, velocity, temperature, and magnetic field by utilizing the global Magnetohydrodynamics (MHD) model as well as the pre-existing gas-dynamic and analytic models. Using this parameterized magnetosheath model, scientists can easily reconstruct expected soft X-ray images and utilize them for analysis of observed images of LEXI and SMILE without simulating the complicated global magnetosphere models. First, we created an MHD based magnetosheath model by running a total of 14 OpenGGCM global MHD simulations under 7 solar wind densities (1, 5, 10, 15, 20, 25, and 30cm−3) and 2 interplanetary magnetic field BZ components (± 4nT), and then parameterizing the results in new magnetosheath conditions. We compared the magnetosheath model result with THEMIS statistical data and it showed good agreement with a weighted Pearson correlation coefficient greater than 0.77, especially for plasma density and plasma velocity. Second, we compiled a suite of magnetosheath models incorporating previous magnetosheath models (gas-dynamic, analytic), and did two case studies to test the performance. The MHD based model was comparable to or better than the previous models while providing self consistency among the magnetosheath parameters. Third, we constructed a tool to calculate a soft X-ray image from any given vantage point, which can support the planning and data analysis of the aforementioned LEXI and SMILE missions. A release of the code has been uploaded to a Github repository.
Document ID
20230014321
Acquisition Source
Goddard Space Flight Center
Document Type
Accepted Manuscript (Version with final changes)
Authors
J. Jung
(University of Maryland, College Park College Park, Maryland, United States)
H. K. Connor
(Goddard Space Flight Center Greenbelt, Maryland, United States)
A.P. Dimmock
(Swedish Institute of Space Physics Kiruna, Sweden)
S. Sembay
(University of Leicester Leicester, United Kingdom)
A.M. Read
(University of Leicester Leicester, United Kingdom)
J. Soucek
(Institute of Atmospheric Physics Prague, Czechia)
Date Acquired
October 2, 2023
Publication Date
December 12, 2023
Publication Information
Publication: Physics of the Earth and Planetary Interiors
Publisher: Elsevier
Volume: 8
Issue Publication Date: December 12, 2023
ISSN: 0031-9201
e-ISSN: 1872-7395
Subject Category
Physics (General)
Funding Number(s)
WBS: 364688.05.18.07.02
CONTRACT_GRANT: 80NSSC21M0180
CONTRACT_GRANT: AGS-1928883
CONTRACT_GRANT: 80NSSC20K1670
CONTRACT_GRANT: 80MSFC20C0019
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
Magnetosheath
Python
Modeling
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