A COMPARISON OF BALMER α ,β, γ EMISSION IN COLLISIONSBETWEEN H+1, H+2, H+3, AND He, Ne, Ar
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Abstract
Balmer α ,β, γ emissions have been measured in collisions between H+1, H+2, H+3, and He, Ne, Ar in energy range of 50-150keV, using TN-1710 optical multichannel analysis system (OMA). The emission cross sections of Hα, Hβ, Hγlines are given. The experimental results demonstrate that the emission cross sections of Hα ,β, γ lines in H+3 +He, Ne, Ar collision systems are larger than those in H+1, H+2 +He , Ne, Ar, respectively.
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PAN Guangyan, LEI Ziming, YANG Feng, LIU Jiarui, YU Dehong, SUN Xiang. A COMPARISON OF BALMER α ,β, γ EMISSION IN COLLISIONSBETWEEN H+1, H+2, H+3, AND He, Ne, Ar[J]. Chin. Phys. Lett., 1989, 6(7): 301-304.
PAN Guangyan, LEI Ziming, YANG Feng, LIU Jiarui, YU Dehong, SUN Xiang. A COMPARISON OF BALMER α ,β, γ EMISSION IN COLLISIONSBETWEEN H+1, H+2, H+3, AND He, Ne, Ar[J]. Chin. Phys. Lett., 1989, 6(7): 301-304.
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PAN Guangyan, LEI Ziming, YANG Feng, LIU Jiarui, YU Dehong, SUN Xiang. A COMPARISON OF BALMER α ,β, γ EMISSION IN COLLISIONSBETWEEN H+1, H+2, H+3, AND He, Ne, Ar[J]. Chin. Phys. Lett., 1989, 6(7): 301-304.
PAN Guangyan, LEI Ziming, YANG Feng, LIU Jiarui, YU Dehong, SUN Xiang. A COMPARISON OF BALMER α ,β, γ EMISSION IN COLLISIONSBETWEEN H+1, H+2, H+3, AND He, Ne, Ar[J]. Chin. Phys. Lett., 1989, 6(7): 301-304.
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