scholarly journals White-Light Continuum Z-scan Technique for Nonlinear Materials Characterization

Author(s):  
M. Balu ◽  
J. Hales ◽  
D.J. Hagan ◽  
E.W. Van Stryland
2004 ◽  
Vol 12 (16) ◽  
pp. 3820 ◽  
Author(s):  
Mihaela Balu ◽  
Joel Hales ◽  
David J. Hagan ◽  
Eric W. Van Stryland

2017 ◽  
Vol 111 (7) ◽  
pp. 071901 ◽  
Author(s):  
Aliasghar Ajami ◽  
Wolfgang Husinsky ◽  
Maximilian Tromayer ◽  
Peter Gruber ◽  
Robert Liska ◽  
...  

2001 ◽  
Vol 18 (3) ◽  
pp. 390-392 ◽  
Author(s):  
Qin Yuan-Dong ◽  
Wang Dan-Ling ◽  
Wang Shu-Feng ◽  
Gong Qi-Huang

2015 ◽  
Vol 379 (34-35) ◽  
pp. 1929-1933 ◽  
Author(s):  
Jiaming Jiang ◽  
Yue Zhong ◽  
Yinghui Zheng ◽  
Zhinan Zeng ◽  
Xiaochun Ge ◽  
...  

2015 ◽  
Vol 11 (S320) ◽  
pp. 268-277
Author(s):  
Arkadiusz Berlicki ◽  
Arun Kumar Awasthi ◽  
Petr Heinzel ◽  
Michal Sobotka

AbstractObservations of flare emissions in the optical continuum are very rare. Therefore, the analysis of such observations is useful and may contribute to our understanding of the flaring chromosphere and photosphere. We study the white light continuum emission observed during the X6.9 flare. This emission comes not only from the flare ribbons but also form the nearby plage area. The main aim of this work is to disentangle the flare and plage (facula) emission. We analyzed the spatial, spectral and temporal evolution of the flare and plage properties by analyzing multi-wavelength observations. We study the morphological correlation of the white-light continuum emission observed with different instruments. We found that some active region areas which produce the continuum emission correspond rather to plages than to the flare kernels. We showed that in some cases the continuum emission from the WL flare kernels is very similar to the continuum emission of faculae.


2015 ◽  
Vol 11 (S320) ◽  
pp. 259-267 ◽  
Author(s):  
Adam F. Kowalski

AbstractIn this talk, we discuss the formation of the near-ultraviolet and optical continuum emission in M dwarf flares through the formation of a dense, heated chromospheric condensation. Results are used from a recent radiative-hydrodynamic model of the response of an M dwarf atmosphere to a high energy flux of nonthermal electrons. These models are used to infer the charge density and optical depth in continuum emitting flare layers from spectra covering the Balmer jump and optical wavelength regimes. Future modeling and observational directions are discussed.


1996 ◽  
Vol 129 (3-4) ◽  
pp. 193-198 ◽  
Author(s):  
A. Brodeur ◽  
F.A. Ilkov ◽  
S.L. Chin

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