Quasistatic Magnetic Field Generation by an Intense Ultrashort Laser Pulse in Underdense Plasma

2000 ◽  
Vol 17 (10) ◽  
pp. 746-748 ◽  
Author(s):  
Zheng Chun-Yang ◽  
Zhu Shao-Ping ◽  
He Xian-Tu
2018 ◽  
Vol 92 (7) ◽  
pp. 919-925 ◽  
Author(s):  
Krishna Gopal ◽  
Md. Ali Raja ◽  
Devki Nandan Gupta ◽  
K. Avinash ◽  
Suresh C. Sharma

1999 ◽  
Vol 59 (1) ◽  
pp. R36-R39 ◽  
Author(s):  
Andrea Macchi ◽  
Enrique Conejero Jarque ◽  
Dieter Bauer ◽  
Fulvio Cornolti ◽  
Luis Plaja

2016 ◽  
Vol 23 (6) ◽  
pp. 063121 ◽  
Author(s):  
A. G. Smyth ◽  
G. Sarri ◽  
M. Vranic ◽  
Y. Amano ◽  
D. Doria ◽  
...  

Optik ◽  
2018 ◽  
Vol 172 ◽  
pp. 437-442
Author(s):  
Sweta Baliyan ◽  
M. Rafat ◽  
Anuraj Panwar ◽  
Vivek Sajal ◽  
C.M. Ryu

2016 ◽  
Vol 380 (16) ◽  
pp. 1437-1441 ◽  
Author(s):  
Mamta Singh ◽  
Krishna Gopal ◽  
Devki Nandan Gupta

1996 ◽  
Vol 14 (1) ◽  
pp. 55-62 ◽  
Author(s):  
V. Yu. Bychenkov ◽  
V.T. Tikhonchuk

The theory of magnetic field generation due to the interaction of short relativistic laser pulses with underdense plasmas has been developed. The magnetic field is generated due to the inverse Faraday effect occurring witha circularly polarized laser pulse. The spatial distribution of the magnetic field is investigated. It is shown that the magnetic field magnitude depends on the relationship between the laser beam radius and the plasma skin-depth.


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