high charge state
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2021 ◽  
Vol 104 (2) ◽  
Author(s):  
Soumya Chatterjee ◽  
Prashant Sharma ◽  
Shashank Singh ◽  
Mumtaz Oswal ◽  
Sunil Kumar ◽  
...  

2020 ◽  
Author(s):  
Tianran Sun

<p>The Earth's magnetosheath is luminous in the soft X-ray band, due to the solar wind charge exchange (SWCX) process. SWCX occurs when a heavy solar wind ion with a high charge state encounters with a neutral component. The heavy ion obtains an electron and gets into an excited state. It then decays to the ground state and emits a photon in the soft X-ray band. Considering that the X-ray emission from the magnetosheath is higher compared to that from the magnetosphere, information about the boundary positions can be derived from an X-ray image of the magnetosheath.</p><p> </p><p>The solar wind - magnetosphere - ionosphere link explorer (SMILE) is a mission jointly supported by ESA and CAS, which aims at exploring the dynamics in the whole system. Soft X-ray Imager (SXI) is expected to provide X-ray images of the magnetosphere. The Modeling Working Group (MWG) is one of the four working groups of SMILE. Studies about the modeling of X-ray emissions as well as the method to derive the boundary positions are two main topics of the MWG. The main progress of MWG will be summarized here. </p>


2019 ◽  
Vol 47 (8) ◽  
pp. 3586-3589 ◽  
Author(s):  
Georgy Yu. Yushkov ◽  
Valeria P. Frolova ◽  
Alexey G. Nikolaev ◽  
Efim M. Oks

2018 ◽  
Author(s):  
A. Efremov ◽  
V. Bekhterev ◽  
S. Bogomolov ◽  
A. Bondarchenko ◽  
A. Lebedev ◽  
...  

2018 ◽  
Author(s):  
T. Thuillier ◽  
L. Maunoury ◽  
J. Angot ◽  
C. Barué ◽  
L. Bonny ◽  
...  

2018 ◽  
Author(s):  
L. Sun ◽  
J. W. Guo ◽  
, Z. Shen ◽  
W. H. Zhang ◽  
X. Z. Zhang ◽  
...  

2017 ◽  
Vol 60 (8) ◽  
pp. 1392-1399 ◽  
Author(s):  
A. S. Bugaev ◽  
A. V. Vizir’ ◽  
V. I. Gushenets ◽  
A. G. Nikolaev ◽  
E. M. Oks ◽  
...  

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