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Mercury Laser Diode Arrays
Barry Freitas, Dave Van Lue, Joe Satariano, Everett Utterbach, Larain DeMercurio, Kurt Cutter, Terry Delima, Ray Beach HAPL Review Crowne Plaza Hotel Pleasanton, CA November 13, 2001 The laser diodes are the pump excitation source for the Mercury Laser system and are critical to its efficient operation. RJB/VG Mercury Laser IFE Meeting 6
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3 backplanes are complete, 4th backplane by December
We have completed the V-BASIS packages for three entire backplanes (>240 kWpeak optical pump power) Split backplane holds 36 V-BASIS tiles 3 backplanes are complete, 4th backplane by December RJB/VG Mercury Laser IFE Meeting 6
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V-BASIS package components
Microlens array and frame Metalized silicon AlN layer Molybdenum base RJB/VG Mercury Laser IFE Meeting 6
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V-BASIS diode tile and plating specifications
V-Groove side of Si, 100 to 200 Å Ti, 10 to 12 µ Ag, 1000 to 1200 Å Ni, 1000 to 1200 Å Au, Top and Bottom of ALN, 1000 to 1200 Å Ti, 6 to 8 µ In, (Top only) Top of Mo Block 6 to 8 µ In, After Si, ALN & Mo parts are assembled 3 to 6 µ In, is deposited on V-Groove side of Si. Bottom side of Si, V-Contacts 6 to 8 µ In, (Bottom only) Shorting Clamp Diode Bars Micro Lens Array AR Coated RJB/VG Mercury Laser IFE Meeting 6
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V-BASIS current flow path
P-Side Connector N-Side P-Side to N-Side Jumper Connector Paddle Shorting Clamp Water Flow Heat Sink Clamping Screws RJB/VG Mercury Laser IFE Meeting 6
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The diode backplane has the required brightness and thermal performance
Fast axis brightness Slow axis brightness The diode backplane provides suitable mechanical tolerance and cooling Intensity RJB/VG Mercury Laser IFE Meeting 6
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Histogram of center wavelengths of 80 fabricated V-BASIS packages
134 amps peak for pulse integrated spectrum and 115 amps for instantaneous chirp measurement Remember, our original modeling specified a gaussian spread with a FWHM of ~ 8 nm. While this distribution is not gaussian it is narrower overall than we had originally anticipated. RJB/VG Mercury Laser IFE Meeting 6
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The V-BASIS packaged diode bars meet the optical specifications of the Mercury Laser System
100 W peak/bar 115 W 44% 2.75 kW (23 bars) Mercury requirement RJB/VG Mercury Laser IFE Meeting 6
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Summary Requirement Status 100 Wpeak/bar 115 Wpeak/bar
Fabrication of 120 tiles (144 tiles per amplifier head) Completed 45% electrical to optical efficiency 44% demonstrated almost Reliability of > 2x108 shots 1.4x108 shots without problems Every package is burned in for 5x106 shots (75 Hz for 18+ hours) Power droop during pulse < 15% 5% droop demonstrated Assemble tiles on split backplane 3 backplanes have been completed, the 4th will be completed by the end of the calendar year Pulse-integrated linewidth < 8.5 nm FWHM Demonstrated 4.7 nm FWHM on tiles for backplane RJB/VG Mercury Laser IFE Meeting 6
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