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Title: X-ray backlighting requirements for the double-shell target

Technical Report ·
DOI:https://doi.org/10.2172/6207946· OSTI ID:6207946

We have analyzed one specific NOVA double-shell target design and have determined the x-ray energies required for probing the performance of the implosion. It is virtually impossible to study the compression of the fuel or the motion of the inner pusher. An x-ray energy of about 9 keV appears to be ideal for measuring the behavior of the outer TaCOH shell for the majority of its travel. However, it would be advantageous to have an x-ray source of about 25 keV to measure the contact between the two shells. Development of narrowband x-ray line sources are more desirable than broadband continuum sources since the intensity per keV is many times greater in the line. Intensities of the probes are determined by the self-emission levels of the target capsule. For the 9 keV line source, an intensity of upwards to 10/sup 15/ keV/keV/sh/cm/sup 2//sr is required with a source area of about 0.01 cm/sup 2/.

Research Organization:
Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
6207946
Report Number(s):
UCID-18773; ON: DE81000241; TRN: 81-017833
Country of Publication:
United States
Language:
English