Development of a new rectangular NaI(Tl) scintillator and spectroscopy of low-energy charged particles

2010 ◽  
Vol 81 (1) ◽  
pp. 013104 ◽  
Author(s):  
Hidehito Nakamura ◽  
Hisashi Kitamura ◽  
Ryuta Hazama
Keyword(s):  
Charged Particles ◽  
Low Energy

Influence of time-variable solar wind on the response of Mercury’s magnetosphere

2021 ◽  
Author(s):  
Sae Aizawa ◽  
Nicolas André ◽  
Ronan Modolo ◽  
Elisabeth Werner ◽  
Jim Slavin ◽  
...  
Keyword(s):  
Magnetic Field ◽  
Solar Wind ◽  
Charged Particles ◽  
Time Variable ◽  
Low Energy ◽  
Field Of View ◽  
Plasma Measurement ◽  
Electrons And Ions ◽  
Low Energy Electrons ◽  
The Magnetic Field

<p><span lang="EN-GB">BepiColombo is going to conduct its first Mercury flyby in October 2021. During this flyby,  plasma measurement will be obtained and bring new insights on the Hermean magnetosphere and its interaction with the Sun despite the limited field of view of the instruments during the cruise phase. Unlike Mariner-10 ion measurements will be obtained, and unlike MESSENGER, low energy electrons and ions will be measured simultaneously. In this study, we have revisited Mariner 10 and MESSENGER observations with the help of the global hybrid model LatHyS in order to understand the influence of time-variable solar wind and to constraint the plasma environment. We are able to reproduce the magnetic field observations of Mariner 10 along its trajectory with in particular two distinct signatures consisting of a quiet and disturbed state of the magnetosphere. In addition, the plasma spectrogram is also collected in the model and this enables us to detail the properties of the charged particles observed during the flyby. We will discuss all these signatures both in term of an interaction with a time-variable solar wind and localized processes occurring in the magnetosphere. We will then present the virtual sampling of both the magnetic field and plasma spectrogram along BepiColombo’s first Mercury flyby trajectory and discuss the possible signatures to be observed at that time.</span></p>

Initial Observations of Low Energy Charged Particles near the Earth’s Bow Shock on ISEE-1

1979 ◽  
pp. 587-595
Author(s):  
F. M. Ipavich ◽  
G. Gloeckler ◽  
C. Y. Fan ◽  
L. A. Fisk ◽  
D. Hovestadt ◽  
...  
Keyword(s):  
Charged Particles ◽  
Bow Shock ◽  
Low Energy ◽  
Earth’S Bow Shock

Acceleration of low energy charged particles by gravitational waves

2006 ◽  
Vol 352 (4-5) ◽  
pp. 261-266 ◽  
Author(s):  
G. Voyatzis ◽  
L. Vlahos ◽  
S. Ichtiaroglou ◽  
D. Papadopoulos
Keyword(s):  
Gravitational Waves ◽  
Charged Particles ◽  
Low Energy

Low energy charged particles in the high latitude heliosphere

1997 ◽  
Vol 19 (6) ◽  
pp. 851-854 ◽  
Author(s):  
L.J. Lanzerotti ◽  
C.G. Maclennan ◽  
T.P. Armstrong ◽  
E.C. Roelof ◽  
R.E. Gold ◽  
...  
Keyword(s):  
High Latitude ◽  
Charged Particles ◽  
Low Energy

scholarly journals A Description of Pseudorapidity Distributions of Charged Particles Produced in Au+Au Collisions at RHIC Energies

2018 ◽  
Vol 2018 ◽  
pp. 1-8
Author(s):  
Z. J. Jiang ◽  
Dongfang Xu ◽  
Yan Huang
Keyword(s):  
Phase Transition ◽  
Heavy Ion Collisions ◽  
Charged Particles ◽  
Dense Matter ◽  
Heavy Ion ◽  
High Energy ◽  
Low Energy ◽  
Ion Collisions ◽  
Rapidity Distributions ◽  
Pseudorapidity Distributions

In heavy ion collisions, charged particles come from two parts: the hot and dense matter and the leading particles. In this paper, the hot and dense matter is assumed to expand according to the hydrodynamic model including phase transition and decouples into particles via the prescription of Cooper-Frye. The leading particles are as usual supposed to have Gaussian rapidity distributions with the number equaling that of participants. The investigations of this paper show that, unlike low energy situations, the leading particles are essential in describing the pseudorapidity distributions of charged particles produced in high energy heavy ion collisions. This might be due to the different transparencies of nuclei at different energies.

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