Thermal Transient Extraction for GaN HEMTs by Frequency-Resolved Gate Resistance Thermometry with Sub-100 ns Time Resolution

2018 ◽  
pp. 1800503
Author(s):  
Adrien Cutivet ◽  
Meriem Bouchilaoun ◽  
Bilal Hassan ◽  
Christophe Rodriguez ◽  
Ali Soltani ◽  
...  
2017 ◽  
Vol 64 (1) ◽  
pp. 78-83 ◽  
Author(s):  
Georges Pavlidis ◽  
Spyridon Pavlidis ◽  
Eric R. Heller ◽  
Elizabeth A. Moore ◽  
Ramakrishna Vetury ◽  
...  

2019 ◽  
Vol 66 (1) ◽  
pp. 330-336 ◽  
Author(s):  
Georges Pavlidis ◽  
Shamit Som ◽  
Jason Barrett ◽  
Wayne Struble ◽  
Samuel Graham

2017 ◽  
Vol 38 (2) ◽  
pp. 240-243 ◽  
Author(s):  
Adrien Cutivet ◽  
Flavien Cozette ◽  
Meriem Bouchilaoun ◽  
Ahmed Chakroun ◽  
Osvaldo Arenas ◽  
...  

Author(s):  
Bryan K. Schwitter ◽  
Anthony E. Parker ◽  
Simon J. Mahon ◽  
Michael C. Heimlich

2018 ◽  
pp. 1800505 ◽  
Author(s):  
Bilal Hassan ◽  
Adrien Cutivet ◽  
Meriem Bouchilaoun ◽  
Christophe Rodriguez ◽  
Ali Soltani ◽  
...  
Keyword(s):  

1994 ◽  
Vol 144 ◽  
pp. 431-434
Author(s):  
M. Minarovjech ◽  
M. Rybanský

AbstractThis paper deals with a possibility to use the ground-based method of observation in order to solve basic problems connected with the solar corona research. Namely:1.heating of the solar corona2.course of the global cycle in the corona3.rotation of the solar corona and development of active regions.There is stressed a possibility of high-time resolution of the coronal line photometer at Lomnický Peak coronal station, and use of the latter to obtain crucial observations.


2000 ◽  
Vol 179 ◽  
pp. 197-200
Author(s):  
Milan Minarovjech ◽  
Milan Rybanský ◽  
Vojtech Rušin

AbstractWe present an analysis of short time-scale intensity variations in the coronal green line as obtained with high time resolution observations. The observed data can be divided into two groups. The first one shows periodic intensity variations with a period of 5 min. the second one does not show any significant intensity variations. We studied the relation between regions of coronal intensity oscillations and the shape of white-light coronal structures. We found that the coronal green-line oscillations occur mainly in regions where open white-light coronal structures are located.


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