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The photoelectron peak at 22–27 eV, a distinctive feature of the energetic electron distribution in the dayside Martian ionosphere, is a useful diagnostic of solar extreme ultraviolet (EUV) and X-ray ionization as well as of large-scale transport along ...
YuTian Cao +3 more
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Response of photoelectron peaks in the Martian ionosphere to solar EUV/X-ray irradiance
An important population of the dayside Martian ionosphere are photoelectrons that are produced by solar Extreme Ultraviolet and X-ray ionization of atmospheric neutrals.
XiaoShu Wu +5 more
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Photoelectron balance in the dayside Martian upper atmosphere
Photoelectrons are produced by solar Extreme Ultraviolet radiation and contribute significantly to the local ionization and heat balances in planetary upper atmospheres. When the effect of transport is negligible, the photoelectron energy distribution is
XiaoShu Wu +4 more
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The \begin{document}$ {\rm{CO}}_2^+$\end{document} ultraviolet doublet (UVD) emission near 289 nm is an important feature of dayside airglow emission from planetary upper atmospheres. In this study, we analyzed the brightness profiles of \begin{document}$
ZiChuan Li +5 more
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Psychological Factors and Reference Potential of Market Mavens
The function of a market maven in the information transfer processes is apparently related to one’s psychological states such as inherent knowledge and involvement level.
Jofi Puspa
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Background Understanding the Mechanism of Action (MoA) of a compound is an often challenging but equally crucial aspect of drug discovery that can help improve both its efficacy and safety.
Layla Hosseini-Gerami +5 more
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Market Mavenism: Its Contribution in Building Consumer’s Trust
In globalization era, firms have to deal with multifaceted challenges. Dynamic changes in consumers’ demands and desires, technology, and new knowledge and innovative movement of competitors are some examples of the important tasks to be managed in order
Jofi Puspa, Conny Tjandra Rahardja
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The Martian bow shock stands as the first defense against the solar wind and shapes the Martian magnetosphere. Previous studies showed the correlation between the Martian bow shock location and solar wind parameters.
Long Cheng +23 more
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Anonymous version of Replication material for our paper under review. THIS VERSION IS "IDENTICAL" TO THE PREVIOUS VERSION REGARDING THE CODE AND MATERIAL. THE ONLY DIFFERENCE IS THAT IN THIS VERSION WE REMOVED THE GITHUB HANDLE OF AUTHORS FROM ALL FILES AND ALSO THE ORGANIZATION NAMES FROM PACKAGE NAMES SO THAT OUR IDENTITY IS NOT ACCIDENTALLY ...
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