Suprathermal energetic electrons and ions generation by an ultraintensive laser pulse in foil plasmas

Author(s):  
T. Okada ◽  
S. Toraya
2004 ◽  
Vol 22 (4) ◽  
pp. 431-438 ◽  
Author(s):  
A.A. ANDREEV ◽  
T. OKADA ◽  
K.Yu. PLATONOV ◽  
S. TORAYA

Analysis and simulations of fast particles produced by a high-intensity short laser pulse interacting with a foil target are performed. Initially, the plasma density distribution of the foil target has a smooth gradient with the scale length of plasma density varying across it. The absorbed laser energy is transferred to fast electrons, which penetrate in the foil and are partially ejected from the foil rear. These electrons produce an electric field that causes an ion beam to be emitted from the foil. We analyze the mechanism of ion acceleration in the foil plasma and the influence of the density gradient and other laser and plasma parameters on ion acceleration. The angular distributions of the ejected electrons and ions are calculated.


Recent progress and future prospects in diagnostics of energetic electrons and ions in the flares are reviewed, together with the roles they play in the flare as a whole. Most of the discussion centres on hard X-ray and gamma-ray and thermal plasma emission data, rather than on radio sources. Since Solar Maximum Mission and Hinotori there has been major progress in all areas of flare electron diagnostics. Electron spectra are now recoverable with some precision, electrons with energies above 10 MeV are known to be highly anisotropic, and indications are available of the spatial distribution of electrons at 20 keV. Timescales of electron acceleration are now known to be shorter than 0.1 s. Energetic electrons are believed to carry much of the flare power. Ion diagnostics are more limited. For greater than 1 MeV ions the flux, spectrum and acceleration timescale are now quite well known. Low energy ions are hard to diagnose but have been invoked as a flare heating mechanism alternative to electron beams. The problems with beam heating models are discussed with special attention to the problems of the low energy proton model and its only direct diagnostic, Hα impact polarization. Finally, theoretical problems associated with return currents and with accelerator requirements are discussed and attention is drawn to the possible importance of entropy as well as energy considerations.


2012 ◽  
Vol 78 (4) ◽  
pp. 497-500 ◽  
Author(s):  
Q.-L. DONG ◽  
D.-W. YUAN ◽  
S.-J. WANG ◽  
Y. T. LI ◽  
X. LIU ◽  
...  

AbstractThe magnetic reconnection (MR) configuration was constructed by using two approaching laser-produced plasma bubbles. The characteristics of the MR current sheet were investigated. The driving energy of the laser pulse affects the type of the current sheet. The experiments present “Y-type” and “X-type” current sheets for larger and smaller driving energy, respectively. The energetic electrons were found to be well-collimated. The formation and ejection of plasmoid from the “Y-type” current sheet was expected to enhance the number of accelerated electrons.


1992 ◽  
Vol 97 (A10) ◽  
pp. 14849 ◽  
Author(s):  
K. Kudela ◽  
D. G. Sibeck ◽  
M. Slivka ◽  
S. Fischer ◽  
V. N. Lutsenko ◽  
...  

1988 ◽  
Vol 93 (A9) ◽  
pp. 9765 ◽  
Author(s):  
B. Hultqvist ◽  
R. Lundin ◽  
K. Stasiewicz ◽  
L. Block ◽  
P.-A. Lindqvist ◽  
...  

2017 ◽  
Vol 147 (1) ◽  
pp. 013942 ◽  
Author(s):  
D. Schomas ◽  
N. Rendler ◽  
J. Krull ◽  
R. Richter ◽  
M. Mudrich

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