Development of a low-energy charged particle detector with on-anode ASIC for in-situ plasma measurement in the Earth’s magnetosphere

2009 ◽  
Author(s):  
M. Saito ◽  
Y. Saito ◽  
T. Mukai ◽  
K. Asamura ◽  
Masfumi Hirahara ◽  
...  
Keyword(s):  
Charged Particle ◽  
Low Energy ◽  
Particle Detector ◽  
Earth’S Magnetosphere ◽  
Plasma Measurement ◽  
Earth's Magnetosphere

scholarly journals First in situ observation of the Moon-originating ions in the Earth's Magnetosphere by MAP-PACE on SELENE (KAGUYA)

2009 ◽  
Vol 36 (22) ◽  
Author(s):  
Takaaki Tanaka ◽  
Yoshifumi Saito ◽  
Shoichiro Yokota ◽  
Kazushi Asamura ◽  
Masaki N. Nishino ◽  
...  
Keyword(s):  
In Situ Observation ◽  
The Moon ◽  
Earth’S Magnetosphere ◽  
Earth's Magnetosphere

Time-resolved measurement of energy loss of low-energy heavy ions in a plasma using a surface-barrier charged-particle detector

2008 ◽  
Vol 50 (2-6) ◽  
pp. 606-610 ◽  
Author(s):  
S. Nishinomiya ◽  
K. Katagiri ◽  
T. Niinou ◽  
J. Kaneko ◽  
H. Fukuda ◽  
...  
Keyword(s):  
Charged Particle ◽  
Energy Loss ◽  
Heavy Ions ◽  
Low Energy ◽  
Surface Barrier ◽  
Particle Detector ◽  
Time Resolved

The SMILE mission: A novel way to explore solar-terrestrial interactions

2020 ◽  
Author(s):  
Graziella Branduardi-Raymont ◽  
Chi Wang ◽  
C. Philippe Escoubet ◽  
Steve Sembay ◽  
Eric Donovan ◽  
...  
Keyword(s):  
Solar Wind ◽  
Spatial Scales ◽  
Current Status ◽  
The Sun ◽  
Earth’S Magnetosphere ◽  
X Ray ◽  
Uv Imaging ◽  
X Ray Imaging ◽  
Earth's Magnetosphere

<p>The coupling between the solar wind and the Earth's magnetosphere-ionosphere system, and the geospace dynamics that result, comprise some of the key questions in space plasma physics. In situ measurements by a fleet of solar wind and magnetospheric missions, current and planned, can provide the most detailed observations of the Sun-Earth connections. However, we are still unable to quantify the global effects of the drivers of such connections, and to monitor their evolution with time. This information is the key missing link for developing a comprehensive understanding of how the Sun gives rise to and controls the Earth's plasma environment and space weather.</p><p>SMILE (Solar wind Magnetosphere Ionosphere Link Explorer) is a novel self-standing mission dedicated to observing the solar wind - magnetosphere coupling via simultaneous X-ray imaging of the magnetosheath and polar cusps (large spatial scales at the magnetopause), UV imaging of global auroral distributions (mesoscale structures in the ionosphere) and in situ solar wind/magnetosheath plasma and magnetic field measurements. X-ray imaging of the magnetosheath and cusps is made possible by the X-ray emission produced in the process of solar wind charge exchange, first observed at comets, and subsequently found to occur in the vicinity of the Earth's magnetosphere. One of the science aims of SMILE is to track the substorm cycle, via X-ray imaging on the dayside and by following its consequences on the nightside with UV imaging. </p><p>SMILE is a collaborative mission between ESA and the Chinese Academy of Sciences (CAS) that was selected in November 2015, adopted into ESA’s Cosmic Vision Programme in March 2019, and is due for launch at the end of 2023. The science that SMILE will deliver, as well as the ongoing technical developments and scientific preparations, and the current status of the mission, will be presented.</p><p> </p>

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