scholarly journals Internally wavelength stabilized 910 nm diode lasers with epitaxially stacked multiple active regions and tunnel junctions

2021 ◽  
Author(s):  
Hans Wenzel ◽  
Jörg Fricke ◽  
Andre Maaßdorf ◽  
Nor Ammouri ◽  
Christof Zink ◽  
...  
2021 ◽  
Author(s):  
Hans Wenzel ◽  
Andre Maaßdorf ◽  
Christof Zink ◽  
Dominik Martin ◽  
Markus Weyers ◽  
...  

Author(s):  
Hari P. Nair ◽  
Rodolfo Salas ◽  
Nathaniel T. Sheehan ◽  
Scott J. Maddox ◽  
Seth R. Bank
Keyword(s):  

2010 ◽  
Vol 18 (2) ◽  
Author(s):  
M. Żujewski ◽  
W. Nakwaski

AbstractThe paper describes an impact of various possible inaccuracies in manufacturing of verticalcavity surface-emitting diode lasers (VCSELs), like thicknesses and compositions of their layers different from assumed ones, on VCSEL room-temperature (RT) continuous-wave (CW) threshold performance. To this end, the fully self-consistent comprehensive optical-electrical-thermal-recombination VCSEL model has been applied. While the analysis has been carried out for the 1.3-μm oxide-confined intra-cavity contacted GaInNAs/GaAs VCSEL, its conclusions are believed to be more general and concern most of modern VCSEL designs. As expected, the VCSEL active region has been found to require the most scrupulous care in its fabrication, any uncontrolled variation in compositions and/or thicknesses of its layers is followed by unaccepted RT CW lasing threshold increase. Also spacer thicknesses should be manufactured with care to ensure a proper overlapping of the optical standing wave and both the gain and lossy areas within the cavity. On the contrary, less than 5% thickness changes in distributed-Bragg-reflectors are followed by nearly insignificant changes in VCSEL RT CW threshold. However, exceeding the above limit causes a rapid increase in lasing thresholds. As expected, in all the above cases, VCSELs equipped with larger active regions have been confirmed to require more careful technology. The above results should enable easier organization of VCSEL manufacturing.


2011 ◽  
Vol 98 (20) ◽  
pp. 201102 ◽  
Author(s):  
C. Gilfert ◽  
V. Ivanov ◽  
N. Oehl ◽  
M. Yacob ◽  
J. P. Reithmaier

1994 ◽  
Vol 144 ◽  
pp. 517-521
Author(s):  
Z. Mouradian ◽  
G. Buchholtz ◽  
G. Zlicaric

AbstractThe synoptic charts of solar rotations 1831 and 1844 have been drawn up, corresponding to the eclipses of 22 July 1990 and 11 July 1991. These charts contain the active regions and the filaments, and show the position of the solar limb, at the time of the eclipse. They are for use in studying the coronal structures observed during these eclipses. The variation of these structures is given in the table. The last section of the article contains a formula for identifying the structures out of the limb.


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