Abstract
Fluorescence emissions from mixtures of Hg with high pressure Xe, Kr, and Ar (∼1 torr Hg, 103–104 torr noble gas) have been studied using a short-pulse relativistic electron beam as an excitation source. Hg–noble gas molecular bands were observed on the red sides of the Hg lines (1849 and 2537 Å) as well as on the red sides of the Hg visible lines (7 3S1→6 3P0,1,2). Temporal histories and production efficiencies of the molecular emissions were determined and a model was formulated for the time histories of the HgXe 2600 Å bands. Possible applications to high power laser systems are discussed.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
