Extreme ultraviolet spectroscopy and modeling of Cu on the SSPX Spheromak and laser plasma “Sparky”

2012 ◽  
Vol 83 (10) ◽  
pp. 10E101 ◽  
Author(s):  
M. E. Weller ◽  
A. S. Safronova ◽  
J. Clementson ◽  
V. L. Kantsyrev ◽  
U. I. Safronova ◽  
...  
Keyword(s):  
Laser Plasma ◽  
Extreme Ultraviolet ◽  
Ultraviolet Spectroscopy

Extreme Ultraviolet Spectroscopy of a Laser Plasma Source for Lithography

1998 ◽  
Vol 57 (2) ◽  
pp. 276-282 ◽  
Author(s):  
A P Shevelko ◽  
L A Shmaenok ◽  
S S Churilov ◽  
R K F J Bastiaensen ◽  
F Bijkerk
Keyword(s):  
Laser Plasma ◽  
Extreme Ultraviolet ◽  
Plasma Source ◽  
Ultraviolet Spectroscopy

Extreme ultraviolet spectroscopy of a laser plasma source for lithography

1997 ◽  
Author(s):  
Fred Bijkerk ◽  
Alexander P. Shevelko ◽  
Leonid A. Shmaenok ◽  
S. S. Churilov
Keyword(s):  
Laser Plasma ◽  
Extreme Ultraviolet ◽  
Plasma Source ◽  
Ultraviolet Spectroscopy

A new method for determining the efficiency of laser radiation conversion into 13.5 ± 0.3 nm radiation in laser-plasma extreme ultraviolet sources

2007 ◽  
Vol 33 (11) ◽  
pp. 945-947 ◽  
Author(s):  
I. V. Domracheva ◽  
M. V. Petrenko ◽  
Z. A. Stepanova ◽  
G. K. Tumakaev ◽  
S. V. Bobashev
Keyword(s):  
Laser Radiation ◽  
Laser Plasma ◽  
Extreme Ultraviolet ◽  
New Method ◽  
Radiation Conversion

scholarly journals Hot phonon and carrier relaxation in Si(100) determined by transient extreme ultraviolet spectroscopy

2018 ◽  
Vol 5 (5) ◽  
pp. 054302 ◽  
Author(s):  
Scott K. Cushing ◽  
Michael Zürch ◽  
Peter M. Kraus ◽  
Lucas M. Carneiro ◽  
Angela Lee ◽  
...  
Keyword(s):  
Extreme Ultraviolet ◽  
Ultraviolet Spectroscopy ◽  
Carrier Relaxation

scholarly journals Extreme Ultraviolet Spectroscopy of Magnetic Cataclysmic Variables

1996 ◽  
Vol 152 ◽  
pp. 309-316
Author(s):  
Frits Paerels ◽  
Min Young Hur ◽  
Christopher W. Mauche
Keyword(s):  
High Resolution ◽  
White Dwarf ◽  
Extreme Ultraviolet ◽  
Cataclysmic Variables ◽  
Ultraviolet Spectroscopy ◽  
Temperature Structure ◽  
Polar Cap ◽  
Ultraviolet Emission ◽  
X Ray ◽  
Magnetic Cataclysmic Variables

A longstanding problem in the interpretation of the X-ray and extreme ultraviolet emission from strongly magnetic cataclysmic variables can be addressed definitively with high resolution EUV spectroscopy. A detailed photospheric spectrum of the accretion-heated polar cap of the white dwarf is sensitive in principle to the temperature structure of the atmosphere. This may allow us to determine where and how the bulk of the accretion energy is thermalized. The EUVE data on AM Herculis and EF Eridani are presented and discussed in this context.

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