2012
DOI: 10.3788/hplpb20122410.2355
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Experimental method for plasma movement in a hole

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Cited by 2 publications
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“…The peak radiation temperature of the hohlraum used was about 180 eV (Ref. 16), and the self-emission of the radiationablated gold plasma was near Planckian with most of its radiation below 1 keV. Even if the plasma collided at the axis of the hole, the photon energy can hardly achieve 2 keV so quickly.…”
Section: Experimental Results and Analysismentioning
confidence: 99%
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“…The peak radiation temperature of the hohlraum used was about 180 eV (Ref. 16), and the self-emission of the radiationablated gold plasma was near Planckian with most of its radiation below 1 keV. Even if the plasma collided at the axis of the hole, the photon energy can hardly achieve 2 keV so quickly.…”
Section: Experimental Results and Analysismentioning
confidence: 99%
“…16 Because CCD counts Aðr; tÞ and XFC spectrum response R(E) [18][19][20] are relative, absolute gold plasma areal density d should be calculated by dividing the CCD counts A 1 , which is generated by the transmitted backlighter radiation through filling gold plasma in the small hole by A 0 , which is generated by direct backlighter radiation…”
Section: Experimental Results and Analysismentioning
confidence: 99%
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